diff --git a/csdown/csharp_prefix.md b/csdown/csharp_prefix.md
index 1b084335..7aa76241 100644
--- a/csdown/csharp_prefix.md
+++ b/csdown/csharp_prefix.md
@@ -123,7 +123,6 @@ these are used in function and type names.
| [Pivot](#Astronomy.Pivot) | Transforms a rotation matrix by pivoting it around a given axis by a given angle. |
| [VectorFromSphere](#Astronomy.VectorFromSphere) | Converts spherical coordinates to Cartesian coordinates. |
| [SphereFromVector](#Astronomy.SphereFromVector) | Converts Cartesian coordinates to spherical coordinates. |
-| [VectorFromEquator](#Astronomy.VectorFromEquator) | Given angular equatorial coordinates, calculates equatorial vector. |
| [EquatorFromVector](#Astronomy.EquatorFromVector) | Given an equatorial vector, calculates equatorial angular coordinates. |
| [VectorFromHorizon](#Astronomy.VectorFromHorizon) | Given apparent angular horizontal coordinates, calculates horizontal vector. |
| [HorizonFromVector](#Astronomy.HorizonFromVector) | Given a vector in horizontal orientation, calculates horizontal angular coordinates. |
diff --git a/demo/browser/astronomy.browser.js b/demo/browser/astronomy.browser.js
index 655b6788..53c40434 100644
--- a/demo/browser/astronomy.browser.js
+++ b/demo/browser/astronomy.browser.js
@@ -35,7 +35,7 @@
'use strict';
Object.defineProperty(exports, "__esModule", { value: true });
exports.SearchPlanetApsis = exports.NextLunarApsis = exports.SearchLunarApsis = exports.Apsis = exports.SearchPeakMagnitude = exports.SearchMaxElongation = exports.Elongation = exports.ElongationEvent = exports.Seasons = exports.SeasonInfo = exports.SearchHourAngle = exports.HourAngleEvent = exports.SearchRiseSet = exports.NextMoonQuarter = exports.SearchMoonQuarter = exports.MoonQuarter = exports.SearchMoonPhase = exports.MoonPhase = exports.SearchRelativeLongitude = exports.Illumination = exports.IlluminationInfo = exports.EclipticLongitude = exports.AngleFromSun = exports.LongitudeFromSun = exports.SearchSunLongitude = exports.Search = exports.GeoVector = exports.HelioDistance = exports.HelioVector = exports.GeoMoon = exports.Ecliptic = exports.Equator = exports.SunPosition = exports.Observer = exports.Horizon = exports.EclipticCoordinates = exports.HorizontalCoordinates = exports.MakeRotation = exports.RotationMatrix = exports.EquatorialCoordinates = exports.Spherical = exports.Vector = exports.CalcMoonCount = exports.MakeTime = exports.AstroTime = exports.SetDeltaTFunction = exports.DeltaT_JplHorizons = exports.DeltaT_EspenakMeeus = exports.Bodies = exports.AngleBetween = void 0;
-exports.NextTransit = exports.SearchTransit = exports.TransitInfo = exports.NextLocalSolarEclipse = exports.SearchLocalSolarEclipse = exports.LocalSolarEclipseInfo = exports.EclipseEvent = exports.NextGlobalSolarEclipse = exports.SearchGlobalSolarEclipse = exports.NextLunarEclipse = exports.GlobalSolarEclipseInfo = exports.SearchLunarEclipse = exports.LunarEclipseInfo = exports.Constellation = exports.ConstellationInfo = exports.Rotation_HOR_ECL = exports.Rotation_ECL_HOR = exports.Rotation_ECL_EQD = exports.Rotation_EQD_ECL = exports.Rotation_EQJ_HOR = exports.Rotation_HOR_EQJ = exports.Rotation_HOR_EQD = exports.Rotation_EQD_HOR = exports.Rotation_EQD_EQJ = exports.Rotation_EQJ_EQD = exports.Rotation_ECL_EQJ = exports.Rotation_EQJ_ECL = exports.RotateVector = exports.InverseRefraction = exports.Refraction = exports.VectorFromHorizon = exports.HorizonFromVector = exports.SphereFromVector = exports.EquatorFromVector = exports.VectorFromEquator = exports.VectorFromSphere = exports.Pivot = exports.IdentityMatrix = exports.CombineRotation = exports.InverseRotation = exports.NextPlanetApsis = void 0;
+exports.NextTransit = exports.SearchTransit = exports.TransitInfo = exports.NextLocalSolarEclipse = exports.SearchLocalSolarEclipse = exports.LocalSolarEclipseInfo = exports.EclipseEvent = exports.NextGlobalSolarEclipse = exports.SearchGlobalSolarEclipse = exports.NextLunarEclipse = exports.GlobalSolarEclipseInfo = exports.SearchLunarEclipse = exports.LunarEclipseInfo = exports.Constellation = exports.ConstellationInfo = exports.Rotation_HOR_ECL = exports.Rotation_ECL_HOR = exports.Rotation_ECL_EQD = exports.Rotation_EQD_ECL = exports.Rotation_EQJ_HOR = exports.Rotation_HOR_EQJ = exports.Rotation_HOR_EQD = exports.Rotation_EQD_HOR = exports.Rotation_EQD_EQJ = exports.Rotation_EQJ_EQD = exports.Rotation_ECL_EQJ = exports.Rotation_EQJ_ECL = exports.RotateVector = exports.InverseRefraction = exports.Refraction = exports.VectorFromHorizon = exports.HorizonFromVector = exports.SphereFromVector = exports.EquatorFromVector = exports.VectorFromSphere = exports.Pivot = exports.IdentityMatrix = exports.CombineRotation = exports.InverseRotation = exports.NextPlanetApsis = void 0;
const DAYS_PER_TROPICAL_YEAR = 365.24217;
const J2000 = new Date('2000-01-01T12:00:00Z');
const PI2 = 2 * Math.PI;
@@ -4658,23 +4658,6 @@ function VectorFromSphere(sphere, time) {
return new Vector(rcoslat * Math.cos(radlon), rcoslat * Math.sin(radlon), sphere.dist * Math.sin(radlat), time);
}
exports.VectorFromSphere = VectorFromSphere;
-/**
- * @brief Given angular equatorial coordinates, calculates the equatorial vector.
- *
- * @param {EquatorialCoordinates} equ
- * An object that contains angular equatorial coordinates to be converted to a vector.
- *
- * @param {AstroTime} time
- * The date and time of the observation. This is needed because the returned
- * vector object requires a valid time value when passed to certain other functions.
- *
- * @returns {Vector}
- * A vector in the equatorial system.
- */
-function VectorFromEquator(equ, time) {
- return VectorFromSphere(new Spherical(equ.dec, 15 * equ.ra, equ.dist), time);
-}
-exports.VectorFromEquator = VectorFromEquator;
/**
* @brief Given an equatorial vector, calculates equatorial angular coordinates.
*
@@ -6160,9 +6143,8 @@ function Constellation(ra, dec) {
Epoch2000 = new AstroTime(0);
}
// Convert coordinates from J2000 to B1875.
- const dummyVector = new Vector(0, 0, 0, Epoch2000); // FIXFIXFIX: rework so we don't need dummy vector
- const equ2000 = new EquatorialCoordinates(ra, dec, 1.0, dummyVector);
- const vec2000 = VectorFromEquator(equ2000, Epoch2000);
+ const sph2000 = new Spherical(dec, 15.0 * ra, 1.0);
+ const vec2000 = VectorFromSphere(sph2000, Epoch2000);
const vec1875 = RotateVector(ConstelRot, vec2000);
const equ1875 = EquatorFromVector(vec1875);
// Search for the constellation using the B1875 coordinates.
diff --git a/demo/nodejs/astronomy.js b/demo/nodejs/astronomy.js
index 7e80d4f3..d49ff1ef 100644
--- a/demo/nodejs/astronomy.js
+++ b/demo/nodejs/astronomy.js
@@ -34,7 +34,7 @@
'use strict';
Object.defineProperty(exports, "__esModule", { value: true });
exports.SearchPlanetApsis = exports.NextLunarApsis = exports.SearchLunarApsis = exports.Apsis = exports.SearchPeakMagnitude = exports.SearchMaxElongation = exports.Elongation = exports.ElongationEvent = exports.Seasons = exports.SeasonInfo = exports.SearchHourAngle = exports.HourAngleEvent = exports.SearchRiseSet = exports.NextMoonQuarter = exports.SearchMoonQuarter = exports.MoonQuarter = exports.SearchMoonPhase = exports.MoonPhase = exports.SearchRelativeLongitude = exports.Illumination = exports.IlluminationInfo = exports.EclipticLongitude = exports.AngleFromSun = exports.LongitudeFromSun = exports.SearchSunLongitude = exports.Search = exports.GeoVector = exports.HelioDistance = exports.HelioVector = exports.GeoMoon = exports.Ecliptic = exports.Equator = exports.SunPosition = exports.Observer = exports.Horizon = exports.EclipticCoordinates = exports.HorizontalCoordinates = exports.MakeRotation = exports.RotationMatrix = exports.EquatorialCoordinates = exports.Spherical = exports.Vector = exports.CalcMoonCount = exports.MakeTime = exports.AstroTime = exports.SetDeltaTFunction = exports.DeltaT_JplHorizons = exports.DeltaT_EspenakMeeus = exports.Bodies = exports.AngleBetween = void 0;
-exports.NextTransit = exports.SearchTransit = exports.TransitInfo = exports.NextLocalSolarEclipse = exports.SearchLocalSolarEclipse = exports.LocalSolarEclipseInfo = exports.EclipseEvent = exports.NextGlobalSolarEclipse = exports.SearchGlobalSolarEclipse = exports.NextLunarEclipse = exports.GlobalSolarEclipseInfo = exports.SearchLunarEclipse = exports.LunarEclipseInfo = exports.Constellation = exports.ConstellationInfo = exports.Rotation_HOR_ECL = exports.Rotation_ECL_HOR = exports.Rotation_ECL_EQD = exports.Rotation_EQD_ECL = exports.Rotation_EQJ_HOR = exports.Rotation_HOR_EQJ = exports.Rotation_HOR_EQD = exports.Rotation_EQD_HOR = exports.Rotation_EQD_EQJ = exports.Rotation_EQJ_EQD = exports.Rotation_ECL_EQJ = exports.Rotation_EQJ_ECL = exports.RotateVector = exports.InverseRefraction = exports.Refraction = exports.VectorFromHorizon = exports.HorizonFromVector = exports.SphereFromVector = exports.EquatorFromVector = exports.VectorFromEquator = exports.VectorFromSphere = exports.Pivot = exports.IdentityMatrix = exports.CombineRotation = exports.InverseRotation = exports.NextPlanetApsis = void 0;
+exports.NextTransit = exports.SearchTransit = exports.TransitInfo = exports.NextLocalSolarEclipse = exports.SearchLocalSolarEclipse = exports.LocalSolarEclipseInfo = exports.EclipseEvent = exports.NextGlobalSolarEclipse = exports.SearchGlobalSolarEclipse = exports.NextLunarEclipse = exports.GlobalSolarEclipseInfo = exports.SearchLunarEclipse = exports.LunarEclipseInfo = exports.Constellation = exports.ConstellationInfo = exports.Rotation_HOR_ECL = exports.Rotation_ECL_HOR = exports.Rotation_ECL_EQD = exports.Rotation_EQD_ECL = exports.Rotation_EQJ_HOR = exports.Rotation_HOR_EQJ = exports.Rotation_HOR_EQD = exports.Rotation_EQD_HOR = exports.Rotation_EQD_EQJ = exports.Rotation_EQJ_EQD = exports.Rotation_ECL_EQJ = exports.Rotation_EQJ_ECL = exports.RotateVector = exports.InverseRefraction = exports.Refraction = exports.VectorFromHorizon = exports.HorizonFromVector = exports.SphereFromVector = exports.EquatorFromVector = exports.VectorFromSphere = exports.Pivot = exports.IdentityMatrix = exports.CombineRotation = exports.InverseRotation = exports.NextPlanetApsis = void 0;
const DAYS_PER_TROPICAL_YEAR = 365.24217;
const J2000 = new Date('2000-01-01T12:00:00Z');
const PI2 = 2 * Math.PI;
@@ -4657,23 +4657,6 @@ function VectorFromSphere(sphere, time) {
return new Vector(rcoslat * Math.cos(radlon), rcoslat * Math.sin(radlon), sphere.dist * Math.sin(radlat), time);
}
exports.VectorFromSphere = VectorFromSphere;
-/**
- * @brief Given angular equatorial coordinates, calculates the equatorial vector.
- *
- * @param {EquatorialCoordinates} equ
- * An object that contains angular equatorial coordinates to be converted to a vector.
- *
- * @param {AstroTime} time
- * The date and time of the observation. This is needed because the returned
- * vector object requires a valid time value when passed to certain other functions.
- *
- * @returns {Vector}
- * A vector in the equatorial system.
- */
-function VectorFromEquator(equ, time) {
- return VectorFromSphere(new Spherical(equ.dec, 15 * equ.ra, equ.dist), time);
-}
-exports.VectorFromEquator = VectorFromEquator;
/**
* @brief Given an equatorial vector, calculates equatorial angular coordinates.
*
@@ -6159,9 +6142,8 @@ function Constellation(ra, dec) {
Epoch2000 = new AstroTime(0);
}
// Convert coordinates from J2000 to B1875.
- const dummyVector = new Vector(0, 0, 0, Epoch2000); // FIXFIXFIX: rework so we don't need dummy vector
- const equ2000 = new EquatorialCoordinates(ra, dec, 1.0, dummyVector);
- const vec2000 = VectorFromEquator(equ2000, Epoch2000);
+ const sph2000 = new Spherical(dec, 15.0 * ra, 1.0);
+ const vec2000 = VectorFromSphere(sph2000, Epoch2000);
const vec1875 = RotateVector(ConstelRot, vec2000);
const equ1875 = EquatorFromVector(vec1875);
// Search for the constellation using the B1875 coordinates.
diff --git a/demo/python/astronomy.py b/demo/python/astronomy.py
index 56978617..8a0c7d1d 100644
--- a/demo/python/astronomy.py
+++ b/demo/python/astronomy.py
@@ -5720,25 +5720,6 @@ def VectorFromSphere(sphere, time):
)
-def VectorFromEquator(equ, time):
- """Given angular equatorial coordinates in `equ`, calculates equatorial vector.
-
- Parameters
- ----------
- equ : Equatorial
- Angular equatorial coordinates to be converted to a vector.
- time : Time
- The date and time of the observation. This is needed because the returned
- vector object requires a valid time value when passed to certain other functions.
-
- Returns
- -------
- Vector
- A vector in the equatorial system.
- """
- return VectorFromSphere(Spherical(equ.dec, 15.0 * equ.ra, equ.dist), time)
-
-
def EquatorFromVector(vec):
"""Given an equatorial vector, calculates equatorial angular coordinates.
@@ -6883,8 +6864,8 @@ def Constellation(ra, dec):
_Epoch2000 = Time(0.0)
# Convert coordinates from J2000 to B1875.
- equ2000 = Equatorial(ra, dec, 1.0, None) # FIXFIXFIX - avoid this hack with unused vector
- vec2000 = VectorFromEquator(equ2000, _Epoch2000)
+ sph2000 = Spherical(dec, 15.0 * ra, 1.0)
+ vec2000 = VectorFromSphere(sph2000, _Epoch2000)
vec1875 = RotateVector(_ConstelRot, vec2000)
equ1875 = EquatorFromVector(vec1875)
diff --git a/generate/ctest.c b/generate/ctest.c
index f35838be..d6c7372e 100644
--- a/generate/ctest.c
+++ b/generate/ctest.c
@@ -2244,7 +2244,7 @@ static int Test_EQJ_EQD(astro_body_t body)
CHECK_STATUS(eqdate);
/* Convert EQJ angular coordinates to vector. */
- v2000 = Astronomy_VectorFromEquator(eq2000, time);
+ v2000 = eq2000.vec;
CHECK_STATUS(v2000);
/* Find rotation matrix. */
@@ -2302,7 +2302,7 @@ static int Test_EQD_HOR(astro_body_t body)
hor = Astronomy_Horizon(&time, observer, eqd.ra, eqd.dec, REFRACTION_NORMAL);
/* Calculate the position of the body as an equatorial vector of date. */
- CHECK_VECTOR(vec_eqd, Astronomy_VectorFromEquator(eqd, time));
+ CHECK_VECTOR(vec_eqd, eqd.vec);
/* Calculate rotation matrix to convert equatorial J2000 vector to horizontal vector. */
rot = Astronomy_Rotation_EQD_HOR(time, observer);
@@ -2321,7 +2321,7 @@ static int Test_EQD_HOR(astro_body_t body)
DEBUG("C Test_EQD_HOR %s: trusted alt=%0.3lf, az=%0.3lf; test alt=%0.3lf, az=%0.3lf; diff_alt=%lg, diff_az=%lg\n",
Astronomy_BodyName(body), hor.altitude, hor.azimuth, sphere.lat, sphere.lon, diff_alt, diff_az);
- if (diff_alt > 3.0e-14 || diff_az > 5e-14)
+ if (diff_alt > 3.0e-14 || diff_az > 7e-14)
FAIL("C Test_EQD_HOR: EXCESSIVE HORIZONTAL ERROR.\n");
/* Confirm that we can convert back to horizontal vector. */
@@ -2342,7 +2342,7 @@ static int Test_EQD_HOR(astro_body_t body)
/* Exercise HOR to EQJ translation. */
CHECK_EQU(eqj, Astronomy_Equator(body, &time, observer, EQUATOR_J2000, ABERRATION));
- CHECK_VECTOR(vec_eqj, Astronomy_VectorFromEquator(eqj, time));
+ CHECK_VECTOR(vec_eqj, eqj.vec);
rot = Astronomy_Rotation_HOR_EQJ(time, observer);
CHECK_ROTMAT(rot);
diff --git a/generate/dotnet/csharp_test/csharp_test.cs b/generate/dotnet/csharp_test/csharp_test.cs
index 09cb23b3..ed6017d7 100644
--- a/generate/dotnet/csharp_test/csharp_test.cs
+++ b/generate/dotnet/csharp_test/csharp_test.cs
@@ -1437,7 +1437,7 @@ namespace csharp_test
var observer = new Observer(35, -85, 0);
Equatorial eq2000 = Astronomy.Equator(body, time, observer, EquatorEpoch.J2000, Aberration.Corrected);
Equatorial eqdate = Astronomy.Equator(body, time, observer, EquatorEpoch.OfDate, Aberration.Corrected);
- AstroVector v2000 = Astronomy.VectorFromEquator(eq2000, time);
+ AstroVector v2000 = eq2000.vec;
RotationMatrix r = Astronomy.Rotation_EQJ_EQD(time);
AstroVector vdate = Astronomy.RotateVector(r, v2000);
Equatorial eqcheck = Astronomy.EquatorFromVector(vdate);
@@ -1474,7 +1474,7 @@ namespace csharp_test
var observer = new Observer(-37.0, +45.0, 0.0);
Equatorial eqd = Astronomy.Equator(body, time, observer, EquatorEpoch.OfDate, Aberration.Corrected);
Topocentric hor = Astronomy.Horizon(time, observer, eqd.ra, eqd.dec, Refraction.Normal);
- AstroVector vec_eqd = Astronomy.VectorFromEquator(eqd, time);
+ AstroVector vec_eqd = eqd.vec;
RotationMatrix rot = Astronomy.Rotation_EQD_HOR(time, observer);
AstroVector vec_hor = Astronomy.RotateVector(rot, vec_eqd);
Spherical sphere = Astronomy.HorizonFromVector(vec_hor, Refraction.Normal);
@@ -1485,7 +1485,7 @@ namespace csharp_test
Debug("C# Test_EQD_HOR {0}: trusted alt={1}, az={2}; test alt={3}, az={4}; diff_alt={5}, diff_az={6}",
body, hor.altitude, hor.azimuth, sphere.lat, sphere.lon, diff_alt, diff_az);
- if (diff_alt > 3.0e-14 || diff_az > 4e-14)
+ if (diff_alt > 3.0e-14 || diff_az > 7.0e-14)
{
Console.WriteLine("C# Test_EQD_HOR: EXCESSIVE HORIZONTAL ERROR.");
return 1;
@@ -1514,7 +1514,7 @@ namespace csharp_test
/* Exercise HOR to EQJ translation. */
Equatorial eqj = Astronomy.Equator(body, time, observer, EquatorEpoch.J2000, Aberration.Corrected);
- AstroVector vec_eqj = Astronomy.VectorFromEquator(eqj, time);
+ AstroVector vec_eqj = eqj.vec;
rot = Astronomy.Rotation_HOR_EQJ(time, observer);
AstroVector check_eqj = Astronomy.RotateVector(rot, vec_hor);
diff --git a/generate/template/astronomy.c b/generate/template/astronomy.c
index e3a1b19b..44f7a087 100644
--- a/generate/template/astronomy.c
+++ b/generate/template/astronomy.c
@@ -5513,36 +5513,6 @@ astro_spherical_t Astronomy_SphereFromVector(astro_vector_t vector)
}
-/**
- * @brief
- * Given angular equatorial coordinates in `equ`, calculates equatorial vector.
- *
- * @param equ
- * Angular equatorial coordinates to be converted to a vector.
- *
- * @param time
- * The date and time of the observation. This is needed because the returned
- * vector requires a valid time value when passed to certain other functions.
- *
- * @return
- * A vector in the equatorial system.
- */
-astro_vector_t Astronomy_VectorFromEquator(astro_equatorial_t equ, astro_time_t time)
-{
- astro_spherical_t sphere;
-
- if (equ.status != ASTRO_SUCCESS)
- return VecError(ASTRO_INVALID_PARAMETER, time);
-
- sphere.status = ASTRO_SUCCESS;
- sphere.lat = equ.dec;
- sphere.lon = 15.0 * equ.ra; /* convert sidereal hours to degrees */
- sphere.dist = equ.dist;
-
- return Astronomy_VectorFromSphere(sphere, time);
-}
-
-
/**
* @brief
* Given an equatorial vector, calculates equatorial angular coordinates.
@@ -5566,6 +5536,7 @@ astro_equatorial_t Astronomy_EquatorFromVector(astro_vector_t vector)
equ.dec = sphere.lat;
equ.ra = sphere.lon / 15.0; /* convert degrees to sidereal hours */
equ.dist = sphere.dist;
+ equ.vec = vector;
return equ;
}
@@ -6195,7 +6166,8 @@ astro_constellation_t Astronomy_Constellation(double ra, double dec)
static astro_time_t epoch2000;
static astro_rotation_t rot = { ASTRO_NOT_INITIALIZED };
astro_constellation_t constel;
- astro_equatorial_t j2000, b1875;
+ astro_spherical_t s2000;
+ astro_equatorial_t b1875;
astro_vector_t vec2000, vec1875;
int i, c;
@@ -6232,11 +6204,11 @@ astro_constellation_t Astronomy_Constellation(double ra, double dec)
}
/* Convert coordinates from J2000 to year 1875. */
- j2000.status = ASTRO_SUCCESS;
- j2000.ra = ra;
- j2000.dec = dec;
- j2000.dist = 1.0;
- vec2000 = Astronomy_VectorFromEquator(j2000, epoch2000);
+ s2000.status = ASTRO_SUCCESS;
+ s2000.lon = ra * 15.0;
+ s2000.lat = dec;
+ s2000.dist = 1.0;
+ vec2000 = Astronomy_VectorFromSphere(s2000, epoch2000);
if (vec2000.status != ASTRO_SUCCESS)
return ConstelErr(vec2000.status);
diff --git a/generate/template/astronomy.cs b/generate/template/astronomy.cs
index 9fc20dfb..c6e5d1ec 100644
--- a/generate/template/astronomy.cs
+++ b/generate/template/astronomy.cs
@@ -6060,20 +6060,6 @@ $ASTRO_IAU_DATA()
}
- /// Given angular equatorial coordinates in `equ`, calculates equatorial vector.
- /// Angular equatorial coordinates to be converted to a vector.
- ///
- /// The date and time of the observation. This is needed because the returned
- /// vector requires a valid time value when passed to certain other functions.
- ///
- /// A vector in the equatorial system.
- public static AstroVector VectorFromEquator(Equatorial equ, AstroTime time)
- {
- var sphere = new Spherical(equ.dec, 15.0 * equ.ra, equ.dist);
- return VectorFromSphere(sphere, time);
- }
-
-
/// Given an equatorial vector, calculates equatorial angular coordinates.
/// A vector in an equatorial coordinate system.
/// Angular coordinates expressed in the same equatorial system as `vector`.
@@ -6675,9 +6661,8 @@ $ASTRO_IAU_DATA()
}
// Convert coordinates from J2000 to B1875.
- var dummyVector = new AstroVector(); // we don't need the vector, but we have to pass one in
- var equ2000 = new Equatorial(ra, dec, 1.0, dummyVector);
- AstroVector vec2000 = VectorFromEquator(equ2000, Epoch2000);
+ var sph2000 = new Spherical(dec, 15.0 * ra, 1.0);
+ AstroVector vec2000 = VectorFromSphere(sph2000, Epoch2000);
AstroVector vec1875 = RotateVector(ConstelRot, vec2000);
Equatorial equ1875 = EquatorFromVector(vec1875);
diff --git a/generate/template/astronomy.py b/generate/template/astronomy.py
index 55762889..be670630 100644
--- a/generate/template/astronomy.py
+++ b/generate/template/astronomy.py
@@ -3823,25 +3823,6 @@ def VectorFromSphere(sphere, time):
)
-def VectorFromEquator(equ, time):
- """Given angular equatorial coordinates in `equ`, calculates equatorial vector.
-
- Parameters
- ----------
- equ : Equatorial
- Angular equatorial coordinates to be converted to a vector.
- time : Time
- The date and time of the observation. This is needed because the returned
- vector object requires a valid time value when passed to certain other functions.
-
- Returns
- -------
- Vector
- A vector in the equatorial system.
- """
- return VectorFromSphere(Spherical(equ.dec, 15.0 * equ.ra, equ.dist), time)
-
-
def EquatorFromVector(vec):
"""Given an equatorial vector, calculates equatorial angular coordinates.
@@ -4535,8 +4516,8 @@ def Constellation(ra, dec):
_Epoch2000 = Time(0.0)
# Convert coordinates from J2000 to B1875.
- equ2000 = Equatorial(ra, dec, 1.0, None) # FIXFIXFIX - avoid this hack with unused vector
- vec2000 = VectorFromEquator(equ2000, _Epoch2000)
+ sph2000 = Spherical(dec, 15.0 * ra, 1.0)
+ vec2000 = VectorFromSphere(sph2000, _Epoch2000)
vec1875 = RotateVector(_ConstelRot, vec2000)
equ1875 = EquatorFromVector(vec1875)
diff --git a/generate/template/astronomy.ts b/generate/template/astronomy.ts
index 6d4649f7..9890c7f7 100644
--- a/generate/template/astronomy.ts
+++ b/generate/template/astronomy.ts
@@ -4205,23 +4205,6 @@ export function VectorFromSphere(sphere: Spherical, time: AstroTime): Vector {
);
}
-/**
- * @brief Given angular equatorial coordinates, calculates the equatorial vector.
- *
- * @param {EquatorialCoordinates} equ
- * An object that contains angular equatorial coordinates to be converted to a vector.
- *
- * @param {AstroTime} time
- * The date and time of the observation. This is needed because the returned
- * vector object requires a valid time value when passed to certain other functions.
- *
- * @returns {Vector}
- * A vector in the equatorial system.
- */
-export function VectorFromEquator(equ: EquatorialCoordinates, time: AstroTime): Vector {
- return VectorFromSphere(new Spherical(equ.dec, 15 * equ.ra, equ.dist), time);
-}
-
/**
* @brief Given an equatorial vector, calculates equatorial angular coordinates.
*
@@ -4855,9 +4838,8 @@ export function Constellation(ra: number, dec: number): ConstellationInfo {
}
// Convert coordinates from J2000 to B1875.
- const dummyVector = new Vector(0, 0, 0, Epoch2000); // FIXFIXFIX: rework so we don't need dummy vector
- const equ2000 = new EquatorialCoordinates(ra, dec, 1.0, dummyVector);
- const vec2000 = VectorFromEquator(equ2000, Epoch2000);
+ const sph2000 = new Spherical(dec, 15.0 * ra, 1.0);
+ const vec2000 = VectorFromSphere(sph2000, Epoch2000);
const vec1875 = RotateVector(ConstelRot, vec2000);
const equ1875 = EquatorFromVector(vec1875);
diff --git a/generate/test.js b/generate/test.js
index c579fcfc..39f7ff99 100644
--- a/generate/test.js
+++ b/generate/test.js
@@ -1282,7 +1282,7 @@ function Rotation() {
const eqdate = Astronomy.Equator(body, time, observer, true, true);
/* Convert EQJ spherical coordinates to vector. */
- const v2000 = Astronomy.VectorFromEquator(eq2000, time);
+ const v2000 = eq2000.vec;
/* Find rotation matrix. */
const r = Astronomy.Rotation_EQJ_EQD(time);
@@ -1319,7 +1319,7 @@ function Rotation() {
const hor = Astronomy.Horizon(time, observer, eqd.ra, eqd.dec, 'normal');
/* Calculate the position of the body as an equatorial vector of date. */
- const vec_eqd = Astronomy.VectorFromEquator(eqd, time);
+ const vec_eqd = eqd.vec;
/* Calculate rotation matrix to convert equatorial J2000 vector to horizontal vector. */
const rot = Astronomy.Rotation_EQD_HOR(time, observer);
@@ -1353,7 +1353,7 @@ function Rotation() {
/* Exercise HOR to EQJ translation. */
const eqj = Astronomy.Equator(body, time, observer, false, true);
- const vec_eqj = Astronomy.VectorFromEquator(eqj, time);
+ const vec_eqj = eqj.vec;
const yrot = Astronomy.Rotation_HOR_EQJ(time, observer);
const check_eqj = Astronomy.RotateVector(yrot, vec_hor);
diff = VectorDiff(check_eqj, vec_eqj);
diff --git a/generate/test.py b/generate/test.py
index 0e3f0ecf..ce87615b 100755
--- a/generate/test.py
+++ b/generate/test.py
@@ -864,7 +864,7 @@ def Test_EQJ_EQD(body):
eqdate = astronomy.Equator(body, time, observer, True, True)
# Convert EQJ spherical coordinates to vector.
- v2000 = astronomy.VectorFromEquator(eq2000, time)
+ v2000 = eq2000.vec
# Find rotation matrix.
r = astronomy.Rotation_EQJ_EQD(time)
@@ -905,7 +905,7 @@ def Test_EQD_HOR(body):
hor = astronomy.Horizon(time, observer, eqd.ra, eqd.dec, astronomy.Refraction.Normal)
# Calculate the position of the body as an equatorial vector of date.
- vec_eqd = astronomy.VectorFromEquator(eqd, time)
+ vec_eqd = eqd.vec
# Calculate rotation matrix to convert equatorial J2000 vector to horizontal vector.
rot = astronomy.Rotation_EQD_HOR(time, observer)
@@ -944,7 +944,7 @@ def Test_EQD_HOR(body):
# Exercise HOR to EQJ translation.
eqj = astronomy.Equator(body, time, observer, False, True)
- vec_eqj = astronomy.VectorFromEquator(eqj, time)
+ vec_eqj = eqj.vec
yrot = astronomy.Rotation_HOR_EQJ(time, observer)
check_eqj = astronomy.RotateVector(yrot, vec_hor)
diff = VectorDiff(check_eqj, vec_eqj)
diff --git a/hydrogen/c_prefix.md b/hydrogen/c_prefix.md
index 01ec74f7..2449df58 100644
--- a/hydrogen/c_prefix.md
+++ b/hydrogen/c_prefix.md
@@ -144,7 +144,6 @@ these are used in function and type names.
| [Pivot](#Astronomy_Pivot) | Transforms a rotation matrix by pivoting it around a given axis by a given angle. |
| [VectorFromSphere](#Astronomy_VectorFromSphere) | Converts spherical coordinates to Cartesian coordinates. |
| [SphereFromVector](#Astronomy_SphereFromVector) | Converts Cartesian coordinates to spherical coordinates. |
-| [VectorFromEquator](#Astronomy_VectorFromEquator) | Given angular equatorial coordinates, calculates equatorial vector. |
| [EquatorFromVector](#Astronomy_EquatorFromVector) | Given an equatorial vector, calculates equatorial angular coordinates. |
| [VectorFromHorizon](#Astronomy_VectorFromHorizon) | Given apparent angular horizontal coordinates, calculates horizontal vector. |
| [HorizonFromVector](#Astronomy_HorizonFromVector) | Given a vector in horizontal orientation, calculates horizontal angular coordinates. |
diff --git a/jsdoc2md/js.hbs b/jsdoc2md/js.hbs
index b9a08558..2bfea80d 100644
--- a/jsdoc2md/js.hbs
+++ b/jsdoc2md/js.hbs
@@ -114,7 +114,6 @@ these are used in function and type names.
| [CombineRotation](#CombineRotation) | Given two rotation matrices, returns a rotation matrix that combines them into a net transformation. |
| [VectorFromSphere](#VectorFromSphere) | Converts spherical coordinates to Cartesian coordinates. |
| [SphereFromVector](#SphereFromVector) | Converts Cartesian coordinates to spherical coordinates. |
-| [VectorFromEquator](#VectorFromEquator) | Given angular equatorial coordinates, calculates equatorial vector. |
| [EquatorFromVector](#EquatorFromVector) | Given an equatorial vector, calculates equatorial angular coordinates. |
| [VectorFromHorizon](#VectorFromHorizon) | Given apparent angular horizontal coordinates, calculates horizontal vector. |
| [HorizonFromVector](#HorizonFromVector) | Given a vector in horizontal orientation, calculates horizontal angular coordinates. |
diff --git a/pydown/py_prefix.md b/pydown/py_prefix.md
index 86bbd9e4..26f23164 100644
--- a/pydown/py_prefix.md
+++ b/pydown/py_prefix.md
@@ -123,7 +123,6 @@ these are used in function and type names.
| [CombineRotation](#CombineRotation) | Given two rotation matrices, returns a rotation matrix that combines them into a net transformation. |
| [VectorFromSphere](#VectorFromSphere) | Converts spherical coordinates to Cartesian coordinates. |
| [SphereFromVector](#SphereFromVector) | Converts Cartesian coordinates to spherical coordinates. |
-| [VectorFromEquator](#VectorFromEquator) | Given angular equatorial coordinates, calculates equatorial vector. |
| [EquatorFromVector](#EquatorFromVector) | Given an equatorial vector, calculates equatorial angular coordinates. |
| [VectorFromHorizon](#VectorFromHorizon) | Given apparent angular horizontal coordinates, calculates horizontal vector. |
| [HorizonFromVector](#HorizonFromVector) | Given a vector in horizontal orientation, calculates horizontal angular coordinates. |
diff --git a/source/c/README.md b/source/c/README.md
index 4f97c6da..f56b08e0 100644
--- a/source/c/README.md
+++ b/source/c/README.md
@@ -144,7 +144,6 @@ these are used in function and type names.
| [Pivot](#Astronomy_Pivot) | Transforms a rotation matrix by pivoting it around a given axis by a given angle. |
| [VectorFromSphere](#Astronomy_VectorFromSphere) | Converts spherical coordinates to Cartesian coordinates. |
| [SphereFromVector](#Astronomy_SphereFromVector) | Converts Cartesian coordinates to spherical coordinates. |
-| [VectorFromEquator](#Astronomy_VectorFromEquator) | Given angular equatorial coordinates, calculates equatorial vector. |
| [EquatorFromVector](#Astronomy_EquatorFromVector) | Given an equatorial vector, calculates equatorial angular coordinates. |
| [VectorFromHorizon](#Astronomy_VectorFromHorizon) | Given apparent angular horizontal coordinates, calculates horizontal vector. |
| [HorizonFromVector](#Astronomy_HorizonFromVector) | Given a vector in horizontal orientation, calculates horizontal angular coordinates. |
@@ -2089,29 +2088,6 @@ After calculating the date and time of an astronomical event in the form of an [
----
-
-
-### Astronomy_VectorFromEquator(equ, time) ⇒ [`astro_vector_t`](#astro_vector_t)
-
-**Given angular equatorial coordinates in `equ`, calculates equatorial vector.**
-
-
-
-
-
-**Returns:** A vector in the equatorial system.
-
-
-
-| Type | Parameter | Description |
-| --- | --- | --- |
-| [`astro_equatorial_t`](#astro_equatorial_t) | `equ` | Angular equatorial coordinates to be converted to a vector. |
-| [`astro_time_t`](#astro_time_t) | `time` | The date and time of the observation. This is needed because the returned vector requires a valid time value when passed to certain other functions. |
-
-
-
-
---
diff --git a/source/c/astronomy.c b/source/c/astronomy.c
index ccb2a73a..2967fa5b 100644
--- a/source/c/astronomy.c
+++ b/source/c/astronomy.c
@@ -6565,36 +6565,6 @@ astro_spherical_t Astronomy_SphereFromVector(astro_vector_t vector)
}
-/**
- * @brief
- * Given angular equatorial coordinates in `equ`, calculates equatorial vector.
- *
- * @param equ
- * Angular equatorial coordinates to be converted to a vector.
- *
- * @param time
- * The date and time of the observation. This is needed because the returned
- * vector requires a valid time value when passed to certain other functions.
- *
- * @return
- * A vector in the equatorial system.
- */
-astro_vector_t Astronomy_VectorFromEquator(astro_equatorial_t equ, astro_time_t time)
-{
- astro_spherical_t sphere;
-
- if (equ.status != ASTRO_SUCCESS)
- return VecError(ASTRO_INVALID_PARAMETER, time);
-
- sphere.status = ASTRO_SUCCESS;
- sphere.lat = equ.dec;
- sphere.lon = 15.0 * equ.ra; /* convert sidereal hours to degrees */
- sphere.dist = equ.dist;
-
- return Astronomy_VectorFromSphere(sphere, time);
-}
-
-
/**
* @brief
* Given an equatorial vector, calculates equatorial angular coordinates.
@@ -6618,6 +6588,7 @@ astro_equatorial_t Astronomy_EquatorFromVector(astro_vector_t vector)
equ.dec = sphere.lat;
equ.ra = sphere.lon / 15.0; /* convert degrees to sidereal hours */
equ.dist = sphere.dist;
+ equ.vec = vector;
return equ;
}
@@ -7702,7 +7673,8 @@ astro_constellation_t Astronomy_Constellation(double ra, double dec)
static astro_time_t epoch2000;
static astro_rotation_t rot = { ASTRO_NOT_INITIALIZED };
astro_constellation_t constel;
- astro_equatorial_t j2000, b1875;
+ astro_spherical_t s2000;
+ astro_equatorial_t b1875;
astro_vector_t vec2000, vec1875;
int i, c;
@@ -7739,11 +7711,11 @@ astro_constellation_t Astronomy_Constellation(double ra, double dec)
}
/* Convert coordinates from J2000 to year 1875. */
- j2000.status = ASTRO_SUCCESS;
- j2000.ra = ra;
- j2000.dec = dec;
- j2000.dist = 1.0;
- vec2000 = Astronomy_VectorFromEquator(j2000, epoch2000);
+ s2000.status = ASTRO_SUCCESS;
+ s2000.lon = ra * 15.0;
+ s2000.lat = dec;
+ s2000.dist = 1.0;
+ vec2000 = Astronomy_VectorFromSphere(s2000, epoch2000);
if (vec2000.status != ASTRO_SUCCESS)
return ConstelErr(vec2000.status);
diff --git a/source/c/astronomy.h b/source/c/astronomy.h
index df26b996..b79a8674 100644
--- a/source/c/astronomy.h
+++ b/source/c/astronomy.h
@@ -876,7 +876,6 @@ astro_rotation_t Astronomy_CombineRotation(astro_rotation_t a, astro_rotation_t
astro_rotation_t Astronomy_Pivot(astro_rotation_t rotation, int axis, double angle);
astro_vector_t Astronomy_VectorFromSphere(astro_spherical_t sphere, astro_time_t time);
astro_spherical_t Astronomy_SphereFromVector(astro_vector_t vector);
-astro_vector_t Astronomy_VectorFromEquator(astro_equatorial_t equ, astro_time_t time);
astro_equatorial_t Astronomy_EquatorFromVector(astro_vector_t vector);
astro_vector_t Astronomy_VectorFromHorizon(astro_spherical_t sphere, astro_time_t time, astro_refraction_t refraction);
astro_spherical_t Astronomy_HorizonFromVector(astro_vector_t vector, astro_refraction_t refraction);
diff --git a/source/csharp/README.md b/source/csharp/README.md
index e91aa8c9..4350f152 100644
--- a/source/csharp/README.md
+++ b/source/csharp/README.md
@@ -123,7 +123,6 @@ these are used in function and type names.
| [Pivot](#Astronomy.Pivot) | Transforms a rotation matrix by pivoting it around a given axis by a given angle. |
| [VectorFromSphere](#Astronomy.VectorFromSphere) | Converts spherical coordinates to Cartesian coordinates. |
| [SphereFromVector](#Astronomy.SphereFromVector) | Converts Cartesian coordinates to spherical coordinates. |
-| [VectorFromEquator](#Astronomy.VectorFromEquator) | Given angular equatorial coordinates, calculates equatorial vector. |
| [EquatorFromVector](#Astronomy.EquatorFromVector) | Given an equatorial vector, calculates equatorial angular coordinates. |
| [VectorFromHorizon](#Astronomy.VectorFromHorizon) | Given apparent angular horizontal coordinates, calculates horizontal vector. |
| [HorizonFromVector](#Astronomy.HorizonFromVector) | Given a vector in horizontal orientation, calculates horizontal angular coordinates. |
@@ -1394,18 +1393,6 @@ In fact, the function [`Astronomy.Seasons`](#Astronomy.Seasons) does use this fu
**Returns:** The ecliptic coordinates of the Sun using the Earth's true equator of date.
-
-### Astronomy.VectorFromEquator(equ, time) ⇒ [`AstroVector`](#AstroVector)
-
-**Given angular equatorial coordinates in `equ`, calculates equatorial vector.**
-
-| Type | Parameter | Description |
-| --- | --- | --- |
-| [`Equatorial`](#Equatorial) | `equ` | Angular equatorial coordinates to be converted to a vector. |
-| [`AstroTime`](#AstroTime) | `time` | The date and time of the observation. This is needed because the returned vector requires a valid time value when passed to certain other functions. |
-
-**Returns:** A vector in the equatorial system.
-
### Astronomy.VectorFromHorizon(sphere, time, refraction) ⇒ [`AstroVector`](#AstroVector)
diff --git a/source/csharp/astronomy.cs b/source/csharp/astronomy.cs
index 618fecee..b7ae9b4f 100644
--- a/source/csharp/astronomy.cs
+++ b/source/csharp/astronomy.cs
@@ -7116,20 +7116,6 @@ namespace CosineKitty
}
- /// Given angular equatorial coordinates in `equ`, calculates equatorial vector.
- /// Angular equatorial coordinates to be converted to a vector.
- ///
- /// The date and time of the observation. This is needed because the returned
- /// vector requires a valid time value when passed to certain other functions.
- ///
- /// A vector in the equatorial system.
- public static AstroVector VectorFromEquator(Equatorial equ, AstroTime time)
- {
- var sphere = new Spherical(equ.dec, 15.0 * equ.ra, equ.dist);
- return VectorFromSphere(sphere, time);
- }
-
-
/// Given an equatorial vector, calculates equatorial angular coordinates.
/// A vector in an equatorial coordinate system.
/// Angular coordinates expressed in the same equatorial system as `vector`.
@@ -7731,9 +7717,8 @@ namespace CosineKitty
}
// Convert coordinates from J2000 to B1875.
- var dummyVector = new AstroVector(); // we don't need the vector, but we have to pass one in
- var equ2000 = new Equatorial(ra, dec, 1.0, dummyVector);
- AstroVector vec2000 = VectorFromEquator(equ2000, Epoch2000);
+ var sph2000 = new Spherical(dec, 15.0 * ra, 1.0);
+ AstroVector vec2000 = VectorFromSphere(sph2000, Epoch2000);
AstroVector vec1875 = RotateVector(ConstelRot, vec2000);
Equatorial equ1875 = EquatorFromVector(vec1875);
diff --git a/source/js/README.md b/source/js/README.md
index a7103621..793de724 100644
--- a/source/js/README.md
+++ b/source/js/README.md
@@ -114,7 +114,6 @@ these are used in function and type names.
| [CombineRotation](#CombineRotation) | Given two rotation matrices, returns a rotation matrix that combines them into a net transformation. |
| [VectorFromSphere](#VectorFromSphere) | Converts spherical coordinates to Cartesian coordinates. |
| [SphereFromVector](#SphereFromVector) | Converts Cartesian coordinates to spherical coordinates. |
-| [VectorFromEquator](#VectorFromEquator) | Given angular equatorial coordinates, calculates equatorial vector. |
| [EquatorFromVector](#EquatorFromVector) | Given an equatorial vector, calculates equatorial angular coordinates. |
| [VectorFromHorizon](#VectorFromHorizon) | Given apparent angular horizontal coordinates, calculates horizontal vector. |
| [HorizonFromVector](#HorizonFromVector) | Given a vector in horizontal orientation, calculates horizontal angular coordinates. |
@@ -1459,21 +1458,6 @@ includes the time, as required by `AstroTime`.
| time | [AstroTime](#AstroTime) | The time that should be included in the returned vector. |
-* * *
-
-
-
-## VectorFromEquator(equ, time) ⇒ [Vector](#Vector)
-**Kind**: global function
-**Returns**: [Vector](#Vector) - A vector in the equatorial system.
-**Brief**: Given angular equatorial coordinates, calculates the equatorial vector.
-
-| Param | Type | Description |
-| --- | --- | --- |
-| equ | [EquatorialCoordinates](#EquatorialCoordinates) | An object that contains angular equatorial coordinates to be converted to a vector. |
-| time | [AstroTime](#AstroTime) | The date and time of the observation. This is needed because the returned vector object requires a valid time value when passed to certain other functions. |
-
-
* * *
diff --git a/source/js/astronomy.browser.js b/source/js/astronomy.browser.js
index 655b6788..53c40434 100644
--- a/source/js/astronomy.browser.js
+++ b/source/js/astronomy.browser.js
@@ -35,7 +35,7 @@
'use strict';
Object.defineProperty(exports, "__esModule", { value: true });
exports.SearchPlanetApsis = exports.NextLunarApsis = exports.SearchLunarApsis = exports.Apsis = exports.SearchPeakMagnitude = exports.SearchMaxElongation = exports.Elongation = exports.ElongationEvent = exports.Seasons = exports.SeasonInfo = exports.SearchHourAngle = exports.HourAngleEvent = exports.SearchRiseSet = exports.NextMoonQuarter = exports.SearchMoonQuarter = exports.MoonQuarter = exports.SearchMoonPhase = exports.MoonPhase = exports.SearchRelativeLongitude = exports.Illumination = exports.IlluminationInfo = exports.EclipticLongitude = exports.AngleFromSun = exports.LongitudeFromSun = exports.SearchSunLongitude = exports.Search = exports.GeoVector = exports.HelioDistance = exports.HelioVector = exports.GeoMoon = exports.Ecliptic = exports.Equator = exports.SunPosition = exports.Observer = exports.Horizon = exports.EclipticCoordinates = exports.HorizontalCoordinates = exports.MakeRotation = exports.RotationMatrix = exports.EquatorialCoordinates = exports.Spherical = exports.Vector = exports.CalcMoonCount = exports.MakeTime = exports.AstroTime = exports.SetDeltaTFunction = exports.DeltaT_JplHorizons = exports.DeltaT_EspenakMeeus = exports.Bodies = exports.AngleBetween = void 0;
-exports.NextTransit = exports.SearchTransit = exports.TransitInfo = exports.NextLocalSolarEclipse = exports.SearchLocalSolarEclipse = exports.LocalSolarEclipseInfo = exports.EclipseEvent = exports.NextGlobalSolarEclipse = exports.SearchGlobalSolarEclipse = exports.NextLunarEclipse = exports.GlobalSolarEclipseInfo = exports.SearchLunarEclipse = exports.LunarEclipseInfo = exports.Constellation = exports.ConstellationInfo = exports.Rotation_HOR_ECL = exports.Rotation_ECL_HOR = exports.Rotation_ECL_EQD = exports.Rotation_EQD_ECL = exports.Rotation_EQJ_HOR = exports.Rotation_HOR_EQJ = exports.Rotation_HOR_EQD = exports.Rotation_EQD_HOR = exports.Rotation_EQD_EQJ = exports.Rotation_EQJ_EQD = exports.Rotation_ECL_EQJ = exports.Rotation_EQJ_ECL = exports.RotateVector = exports.InverseRefraction = exports.Refraction = exports.VectorFromHorizon = exports.HorizonFromVector = exports.SphereFromVector = exports.EquatorFromVector = exports.VectorFromEquator = exports.VectorFromSphere = exports.Pivot = exports.IdentityMatrix = exports.CombineRotation = exports.InverseRotation = exports.NextPlanetApsis = void 0;
+exports.NextTransit = exports.SearchTransit = exports.TransitInfo = exports.NextLocalSolarEclipse = exports.SearchLocalSolarEclipse = exports.LocalSolarEclipseInfo = exports.EclipseEvent = exports.NextGlobalSolarEclipse = exports.SearchGlobalSolarEclipse = exports.NextLunarEclipse = exports.GlobalSolarEclipseInfo = exports.SearchLunarEclipse = exports.LunarEclipseInfo = exports.Constellation = exports.ConstellationInfo = exports.Rotation_HOR_ECL = exports.Rotation_ECL_HOR = exports.Rotation_ECL_EQD = exports.Rotation_EQD_ECL = exports.Rotation_EQJ_HOR = exports.Rotation_HOR_EQJ = exports.Rotation_HOR_EQD = exports.Rotation_EQD_HOR = exports.Rotation_EQD_EQJ = exports.Rotation_EQJ_EQD = exports.Rotation_ECL_EQJ = exports.Rotation_EQJ_ECL = exports.RotateVector = exports.InverseRefraction = exports.Refraction = exports.VectorFromHorizon = exports.HorizonFromVector = exports.SphereFromVector = exports.EquatorFromVector = exports.VectorFromSphere = exports.Pivot = exports.IdentityMatrix = exports.CombineRotation = exports.InverseRotation = exports.NextPlanetApsis = void 0;
const DAYS_PER_TROPICAL_YEAR = 365.24217;
const J2000 = new Date('2000-01-01T12:00:00Z');
const PI2 = 2 * Math.PI;
@@ -4658,23 +4658,6 @@ function VectorFromSphere(sphere, time) {
return new Vector(rcoslat * Math.cos(radlon), rcoslat * Math.sin(radlon), sphere.dist * Math.sin(radlat), time);
}
exports.VectorFromSphere = VectorFromSphere;
-/**
- * @brief Given angular equatorial coordinates, calculates the equatorial vector.
- *
- * @param {EquatorialCoordinates} equ
- * An object that contains angular equatorial coordinates to be converted to a vector.
- *
- * @param {AstroTime} time
- * The date and time of the observation. This is needed because the returned
- * vector object requires a valid time value when passed to certain other functions.
- *
- * @returns {Vector}
- * A vector in the equatorial system.
- */
-function VectorFromEquator(equ, time) {
- return VectorFromSphere(new Spherical(equ.dec, 15 * equ.ra, equ.dist), time);
-}
-exports.VectorFromEquator = VectorFromEquator;
/**
* @brief Given an equatorial vector, calculates equatorial angular coordinates.
*
@@ -6160,9 +6143,8 @@ function Constellation(ra, dec) {
Epoch2000 = new AstroTime(0);
}
// Convert coordinates from J2000 to B1875.
- const dummyVector = new Vector(0, 0, 0, Epoch2000); // FIXFIXFIX: rework so we don't need dummy vector
- const equ2000 = new EquatorialCoordinates(ra, dec, 1.0, dummyVector);
- const vec2000 = VectorFromEquator(equ2000, Epoch2000);
+ const sph2000 = new Spherical(dec, 15.0 * ra, 1.0);
+ const vec2000 = VectorFromSphere(sph2000, Epoch2000);
const vec1875 = RotateVector(ConstelRot, vec2000);
const equ1875 = EquatorFromVector(vec1875);
// Search for the constellation using the B1875 coordinates.
diff --git a/source/js/astronomy.browser.min.js b/source/js/astronomy.browser.min.js
index a4823cdc..2db50220 100644
--- a/source/js/astronomy.browser.min.js
+++ b/source/js/astronomy.browser.min.js
@@ -36,16 +36,16 @@ $jscomp.polyfillIsolated=function(p,t,h,x){var r=p.split(".");p=1===r.length;x=r
$jscomp.POLYFILL_PREFIX+r),$jscomp.defineProperty(x,$jscomp.propertyToPolyfillSymbol[r],{configurable:!0,writable:!0,value:t})))};$jscomp.polyfill("Math.log10",function(p){return p?p:function(t){return Math.log(t)/Math.LN10}},"es6","es3");$jscomp.polyfill("Number.isFinite",function(p){return p?p:function(t){return"number"!==typeof t?!1:!isNaN(t)&&Infinity!==t&&-Infinity!==t}},"es6","es3");$jscomp.polyfill("Number.MAX_SAFE_INTEGER",function(){return 9007199254740991},"es6","es3");
$jscomp.polyfill("Number.isInteger",function(p){return p?p:function(t){return Number.isFinite(t)?t===Math.floor(t):!1}},"es6","es3");$jscomp.polyfill("Number.isSafeInteger",function(p){return p?p:function(t){return Number.isInteger(t)&&Math.abs(t)<=Number.MAX_SAFE_INTEGER}},"es6","es3");
(function(p){"object"===typeof exports&&"undefined"!==typeof module?module.exports=p():"function"===typeof define&&define.amd?define([],p):("undefined"!==typeof window?window:"undefined"!==typeof global?global:"undefined"!==typeof self?self:this).Astronomy=p()})(function(){return function(){function p(t,h,x){function r(J,L){if(!h[J]){if(!t[J]){var y="function"==typeof require&&require;if(!L&&y)return y(J,!0);if(I)return I(J,!0);L=Error("Cannot find module '"+J+"'");throw L.code="MODULE_NOT_FOUND",
-L;}L=h[J]={exports:{}};t[J][0].call(L.exports,function(oa){return r(t[J][1][oa]||oa)},L,L.exports,p,t,h,x)}return h[J].exports}for(var I="function"==typeof require&&require,O=0;OMath.abs(c))throw"AngleBetween: first vector is too short.";var d=b.x*b.x+b.y*b.y+b.z*b.z;if(1E-8>Math.abs(d))throw"AngleBetween: second vector is too short.";a=(a.x*b.x+a.y*b.y+a.z*b.z)/Math.sqrt(c*d);return-1>=a?180:1<=a?0:57.29577951308232*Math.acos(a)}function J(a){var b=2E3+(a-14)/365.24217;if(-500>b)return a=(b-1820)/100,-20+32*a*a;if(500>b){a=b/100;b=a*a;var c=a*b;return 10583.6-1014.41*a+33.78311*b-5.952053*c-.1798452*b*b+.022174192*b*c+.0090316521*c*c}if(1600>b)return a=
(b-1E3)/100,b=a*a,c=a*b,1574.2-556.01*a+71.23472*b+.319781*c-.8503463*b*b-.005050998*b*c+.0083572073*c*c;if(1700>b)return a=b-1600,b=a*a,120-.9808*a-.01532*b+a*b/7129;if(1800>b)return a=b-1700,b=a*a,8.83+.1603*a-.0059285*b+1.3336E-4*a*b-b*b/1174E3;if(1860>b){a=b-1800;b=a*a;c=a*b;var d=b*b;return 13.72-.332447*a+.0068612*b+.0041116*c-3.7436E-4*d+1.21272E-5*b*c-1.699E-7*c*c+8.75E-10*c*d}if(1900>b)return a=b-1860,b=a*a,c=a*b,7.62+.5737*a-.251754*b+.01680668*c-4.473624E-4*b*b+b*c/233174;if(1920>b)return a=
b-1900,b=a*a,-2.79+1.494119*a-.0598939*b+.0061966*a*b-1.97E-4*b*b;if(1941>b)return a=b-1920,b=a*a,21.2+.84493*a-.0761*b+.0020936*a*b;if(1961>b)return a=b-1950,b=a*a,29.07+.407*a-b/233+a*b/2547;if(1986>b)return a=b-1975,b=a*a,45.45+1.067*a-b/260-a*b/718;if(2005>b)return a=b-2E3,b=a*a,c=a*b,63.86+.3345*a-.060374*b+.0017275*c+6.51814E-4*b*b+2.373599E-5*b*c;if(2050>b)return a=b-2E3,62.92+.32217*a+.005589*a*a;if(2150>b)return a=(b-1820)/100,-20+32*a*a-.5628*(2150-b);a=(b-1820)/100;return-20+32*a*a}function L(a){return a+
-sb(a)/86400}function y(a){return a instanceof P?a:new P(a)}function oa(a){a=a.tt/36525;return(((((-4.34E-8*a-5.76E-7)*a+.0020034)*a-1.831E-4)*a-46.836769)*a+84381.406)/3600}function Ca(a){var b;if(!Da||1E-6=A;++A)0!==v[A]&&f(D.x,D.y,c(w,v[A],A),c(H,v[A],A),function(Z,fa){return D.x=Z,D.y=fa});return D}function g(v,A,G,T,D,Z,fa,Va){D=l(D,Z,fa,Va);q+=v*D.y;u+=A*D.y;wb+=G*D.x;xb+=T*D.x}++h.CalcMoonCount;a=a.tt/36525;var m,n,q,u,w=b(-6,6,1,4),H=b(-6,6,1,4);var z=a*a;var wb=u=q=0;var xb=3422.7;var aa=k(.19833+.05611*a);var U=k(.27869+.04508*a);var M=k(.16827-.36903*a);var R=k(.34734-5.37261*a);var pa=k(.10498-5.37899*a);var Ea=k(.42681-.41855*a),wc=k(.14943-5.37511*a);var Fa=.84*aa+.31*U+
-14.27*M+7.26*R+.28*pa+.24*Ea;var Xa=2.94*aa+.31*U+14.27*M+9.34*R+1.12*pa+.83*Ea;var Ga=-6.4*aa-1.89*Ea;U=.21*aa+.31*U+14.27*M-88.7*R-15.3*pa+.24*Ea-1.86*wc;M=Fa-Ga;aa=-3.332E-6*k(.59734-5.37261*a)-5.39E-7*k(.35498-5.37899*a)-6.4E-8*k(.39943-5.37511*a);Fa=Q*I(.60643382+1336.85522467*a-3.13E-6*z)+Fa/V;Xa=Q*I(.37489701+1325.55240982*a+2.565E-5*z)+Xa/V;Ga=Q*I(.99312619+99.99735956*a-4.4E-7*z)+Ga/V;U=Q*I(.25909118+1342.2278298*a-8.92E-6*z)+U/V;pa=Q*I(.82736186+1236.85308708*a-3.97E-6*z)+M/V;for(m=1;4>=
-m;++m){switch(m){case 1:M=Xa;z=4;R=1.000002208;break;case 2:M=Ga;z=3;R=.997504612-.002495388*a;break;case 3:M=U;z=4;R=1.000002708+139.978*aa;break;case 4:M=pa;z=6;R=1;break;default:throw"Internal error: I = "+m;}d(0,m,1);d(1,m,Math.cos(M)*R);e(0,m,0);e(1,m,Math.sin(M)*R);for(n=2;n<=z;++n)f(c(w,n-1,m),c(H,n-1,m),c(w,1,m),c(H,1,m),function(v,A){return d(n,m,v),e(n,m,A)});for(n=1;n<=z;++n)d(-n,m,c(w,n,m)),e(-n,m,-c(H,n,m))}g(13.902,14.06,-.001,.2607,0,0,0,4);g(.403,-4.01,.394,.0023,0,0,0,3);g(2369.912,
+rb(a)/86400}function y(a){return a instanceof P?a:new P(a)}function na(a){a=a.tt/36525;return(((((-4.34E-8*a-5.76E-7)*a+.0020034)*a-1.831E-4)*a-46.836769)*a+84381.406)/3600}function Ca(a){var b;if(!Da||1E-6=A;++A)0!==v[A]&&f(D.x,D.y,c(w,v[A],A),c(H,v[A],A),function(Z,fa){return D.x=Z,D.y=fa});return D}function g(v,A,G,T,D,Z,fa,Va){D=l(D,Z,fa,Va);q+=v*D.y;u+=A*D.y;vb+=G*D.x;wb+=T*D.x}++h.CalcMoonCount;a=a.tt/36525;var m,n,q,u,w=b(-6,6,1,4),H=b(-6,6,1,4);var z=a*a;var vb=u=q=0;var wb=3422.7;var aa=k(.19833+.05611*a);var U=k(.27869+.04508*a);var M=k(.16827-.36903*a);var R=k(.34734-5.37261*a);var oa=k(.10498-5.37899*a);var Ea=k(.42681-.41855*a),vc=k(.14943-5.37511*a);var Fa=.84*aa+.31*U+
+14.27*M+7.26*R+.28*oa+.24*Ea;var Xa=2.94*aa+.31*U+14.27*M+9.34*R+1.12*oa+.83*Ea;var Ga=-6.4*aa-1.89*Ea;U=.21*aa+.31*U+14.27*M-88.7*R-15.3*oa+.24*Ea-1.86*vc;M=Fa-Ga;aa=-3.332E-6*k(.59734-5.37261*a)-5.39E-7*k(.35498-5.37899*a)-6.4E-8*k(.39943-5.37511*a);Fa=Q*I(.60643382+1336.85522467*a-3.13E-6*z)+Fa/V;Xa=Q*I(.37489701+1325.55240982*a+2.565E-5*z)+Xa/V;Ga=Q*I(.99312619+99.99735956*a-4.4E-7*z)+Ga/V;U=Q*I(.25909118+1342.2278298*a-8.92E-6*z)+U/V;oa=Q*I(.82736186+1236.85308708*a-3.97E-6*z)+M/V;for(m=1;4>=
+m;++m){switch(m){case 1:M=Xa;z=4;R=1.000002208;break;case 2:M=Ga;z=3;R=.997504612-.002495388*a;break;case 3:M=U;z=4;R=1.000002708+139.978*aa;break;case 4:M=oa;z=6;R=1;break;default:throw"Internal error: I = "+m;}d(0,m,1);d(1,m,Math.cos(M)*R);e(0,m,0);e(1,m,Math.sin(M)*R);for(n=2;n<=z;++n)f(c(w,n-1,m),c(H,n-1,m),c(w,1,m),c(H,1,m),function(v,A){return d(n,m,v),e(n,m,A)});for(n=1;n<=z;++n)d(-n,m,c(w,n,m)),e(-n,m,-c(H,n,m))}g(13.902,14.06,-.001,.2607,0,0,0,4);g(.403,-4.01,.394,.0023,0,0,0,3);g(2369.912,
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0,1,0,1);g(-668.146,-126.98,-1.302,-.3997,0,1,0,0);g(.56,.32,-.001,-.0037,0,1,0,-1);g(-165.145,-165.06,.054,1.9178,0,1,0,-2);g(-1.877,-6.46,-.416,.0339,0,1,0,-4);g(.213,1.02,-.074,.0054,2,0,0,4);g(14.387,14.78,-.017,.2833,2,0,0,2);g(-.586,-1.2,.054,-.01,2,0,0,1);g(769.016,767.96,.107,10.1657,2,0,0,0);g(1.75,2.01,-.018,.0155,2,0,0,-1);g(-211.656,-152.53,5.679,-.3039,2,0,0,-2);g(1.225,.91,-.03,-.0088,2,0,0,-3);g(-30.773,-34.07,-.308,.3722,2,0,0,-4);g(-.57,-1.4,-.074,.0109,2,0,0,-6);g(-2.921,-11.75,
.787,-.0484,1,1,0,2);g(1.267,1.52,-.022,.0164,1,1,0,1);g(-109.673,-115.18,.461,-.949,1,1,0,0);g(-205.962,-182.36,2.056,1.4437,1,1,0,-2);g(.233,.36,.012,-.0025,1,1,0,-3);g(-4.391,-9.66,-.471,.0673,1,1,0,-4);g(.283,1.53,-.111,.006,1,-1,0,4);g(14.577,31.7,-1.54,.2302,1,-1,0,2);g(147.687,138.76,.679,1.1528,1,-1,0,0);g(-1.089,.55,.021,0,1,-1,0,-1);g(28.475,23.59,-.443,-.2257,1,-1,0,-2);g(-.276,-.38,-.006,-.0036,1,-1,0,-3);g(.636,2.27,.146,-.0102,1,-1,0,-4);g(-.189,-1.68,.131,-.0028,0,2,0,2);g(-7.486,-.66,
@@ -54,56 +54,56 @@ m;++m){switch(m){case 1:M=Xa;z=4;R=1.000002208;break;case 2:M=Ga;z=3;R=.99750461
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3,1,0,-2);g(.681,.96,-.026,.0115,3,-1,0,0);g(-.297,-.27,.002,-9E-4,2,2,0,-2);g(.254,.21,-.003,0,2,-2,0,-2);g(-.25,-.22,.004,.0014,1,3,0,-2);g(-3.996,0,0,4E-4,2,0,2,0);g(.557,-.75,0,-.009,2,0,2,-2);g(-.459,-.38,0,-.0053,2,0,-2,2);g(-1.298,.74,0,4E-4,2,0,-2,0);g(.538,1.14,0,-.0141,2,0,-2,-2);g(.263,.02,0,0,1,1,2,0);g(.426,.07,0,-6E-4,1,1,-2,-2);g(-.304,.03,0,3E-4,1,-1,2,0);g(-.372,-.19,0,-.0027,1,-1,-2,2);g(.418,0,0,0,0,0,4,0);g(-.33,-.04,0,0,3,0,2,0);z=-526.069*l(0,0,1,-2).y;z+=-3.352*l(0,0,1,-4).y;
z+=44.297*l(1,0,1,-2).y;z+=-6*l(1,0,1,-4).y;z+=20.599*l(-1,0,1,0).y;z+=-30.598*l(-1,0,1,-2).y;z+=-24.649*l(-2,0,1,0).y;z+=-2*l(-2,0,1,-2).y;z+=-22.571*l(0,1,1,-2).y;z+=10.985*l(0,-1,1,-2).y;q+=.82*k(.7736-62.5512*a)+.31*k(.0466-125.1025*a)+.35*k(.5785-25.1042*a)+.66*k(.4591+1335.8075*a)+.64*k(.313-91.568*a)+1.14*k(.148+1331.2898*a)+.21*k(.5918+1056.5859*a)+.44*k(.5784+1322.8595*a)+.24*k(.2275-5.7374*a)+.28*k(.2965+2.6929*a)+.33*k(.3132+6.3368*a);a=U+u/V;a=(1.000002708+139.978*aa)*(18518.511+1.189+
-wb)*Math.sin(a)-6.24*Math.sin(3*a)+z;return{geo_eclip_lon:Q*I((Fa+q/V)/Q),geo_eclip_lat:Math.PI/648E3*a,distance_au:4.263520978299708E-5*V/(.999953253*xb)}}function Ha(a,b,c){a=Ya(a,c);return[a.rot[0][0]*b[0]+a.rot[1][0]*b[1]+a.rot[2][0]*b[2],a.rot[0][1]*b[0]+a.rot[1][1]*b[1]+a.rot[2][1]*b[2],a.rot[0][2]*b[0]+a.rot[1][2]*b[1]+a.rot[2][2]*b[2]]}function Ya(a,b){var c=84381.406;if(0!==a&&0!==b)throw"One of (tt1, tt2) must be 0.";a=(b-a)/36525;0===b&&(a=-a);var d=((((3.337E-7*a-4.67E-7)*a-.00772503)*
+vb)*Math.sin(a)-6.24*Math.sin(3*a)+z;return{geo_eclip_lon:Q*I((Fa+q/V)/Q),geo_eclip_lat:Math.PI/648E3*a,distance_au:4.263520978299708E-5*V/(.999953253*wb)}}function Ha(a,b,c){a=Ya(a,c);return[a.rot[0][0]*b[0]+a.rot[1][0]*b[1]+a.rot[2][0]*b[2],a.rot[0][1]*b[0]+a.rot[1][1]*b[1]+a.rot[2][1]*b[2],a.rot[0][2]*b[0]+a.rot[1][2]*b[1]+a.rot[2][2]*b[2]]}function Ya(a,b){var c=84381.406;if(0!==a&&0!==b)throw"One of (tt1, tt2) must be 0.";a=(b-a)/36525;0===b&&(a=-a);var d=((((3.337E-7*a-4.67E-7)*a-.00772503)*
a+.0512623)*a-.025754)*a+c;c*=4.84813681109536E-6;var e=((((-9.51E-8*a+1.32851E-4)*a-.00114045)*a-1.0790069)*a+5038.481507)*a*4.84813681109536E-6;d*=4.84813681109536E-6;var f=((((-5.6E-8*a+1.70663E-4)*a-.00121197)*a-2.3814292)*a+10.556403)*a*4.84813681109536E-6;a=Math.sin(c);c=Math.cos(c);var k=Math.sin(-e);e=Math.cos(-e);var l=Math.sin(-d);var g=Math.cos(-d);var m=Math.sin(f);var n=Math.cos(f);f=n*e-k*m*g;d=n*k*c+m*g*e*c-a*m*l;var q=n*k*a+m*g*e*a+c*m*l;var u=-m*e-k*n*g;var w=-m*k*c+n*g*e*c-a*n*l;
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-a[1],a[2],b);var c=b.x*b.x+b.y*b.y,d=Math.sqrt(c+b.z*b.z);if(0===c){if(0===b.z)throw"Indeterminate sky coordinates";return 0>b.z?new ha(0,-90,d,b):new ha(0,90,d,b)}var e=Math.atan2(b.y,b.x)/.2617993877991494;0>e&&(e+=24);return new ha(e,Math.atan2(a[2],Math.sqrt(c))/.017453292519943295,d,b)}function ia(a,b){var c=.017453292519943295*a;a=Math.cos(c);c=Math.sin(c);return[a*b[0]+c*b[1]+0*b[2],-c*b[0]+a*b[1]+0*b[2],0*b[0]+0*b[1]+1*b[2]]}function Ia(a,b,c,d,e){a=y(a);ja(b);r(c);r(d);var f=Math.sin(.017453292519943295*
-b.latitude),k=Math.cos(.017453292519943295*b.latitude),l=Math.sin(.017453292519943295*b.longitude),g=Math.cos(.017453292519943295*b.longitude);b=Math.sin(.017453292519943295*d);var m=Math.cos(.017453292519943295*d),n=Math.sin(.2617993877991494*c),q=Math.cos(.2617993877991494*c),u=[k*g,k*l,f];f=[-f*g,-f*l,k];l=[l,-g,0];k=-15*qa(a);a=ia(k,u);u=ia(k,f);l=ia(k,l);b=[m*q,m*n,b];n=b[0]*a[0]+b[1]*a[1]+b[2]*a[2];m=b[0]*u[0]+b[1]*u[1]+b[2]*u[2];u=b[0]*l[0]+b[1]*l[1]+b[2]*l[2];q=Math.sqrt(m*m+u*u);0m&&(m+=360)):m=0;n=57.29577951308232*Math.atan2(q,n);q=d;if(e&&(d=n,e=ra(e,90-n),n-=e,0l;++l)e.push((b[l]-d*a[l])/u*c+a[l]*q);q=Math.sqrt(e[0]*e[0]+e[1]*e[1]);0c&&(c+=24)):c=0;q=57.29577951308232*Math.atan2(e[2],q)}return new Ab(m,90-n,c,q)}function ja(a){if(!(a instanceof
-Bb))throw"Not an instance of the Observer class: "+a;r(a.latitude);r(a.longitude);r(a.height);if(-90>a.latitude||90d&&(d+=360));return new Eb(a,f,b,57.29577951308232*Math.atan2(b,c),d)}function sa(a,b,c){void 0===Ka&&(Ka=.017453292519943295*Ca(y(ab)).mobl,Fb=Math.cos(Ka),Gb=Math.sin(Ka));r(a);r(b);r(c);return Db(a,b,c,Fb,Gb)}function X(a){a=y(a);var b=S(a),c=b.distance_au*
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+a[1],a[2],b);var c=b.x*b.x+b.y*b.y,d=Math.sqrt(c+b.z*b.z);if(0===c){if(0===b.z)throw"Indeterminate sky coordinates";return 0>b.z?new qa(0,-90,d,b):new qa(0,90,d,b)}var e=Math.atan2(b.y,b.x)/.2617993877991494;0>e&&(e+=24);return new qa(e,Math.atan2(a[2],Math.sqrt(c))/.017453292519943295,d,b)}function ha(a,b){var c=.017453292519943295*a;a=Math.cos(c);c=Math.sin(c);return[a*b[0]+c*b[1]+0*b[2],-c*b[0]+a*b[1]+0*b[2],0*b[0]+0*b[1]+1*b[2]]}function Ia(a,b,c,d,e){a=y(a);ia(b);r(c);r(d);var f=Math.sin(.017453292519943295*
+b.latitude),k=Math.cos(.017453292519943295*b.latitude),l=Math.sin(.017453292519943295*b.longitude),g=Math.cos(.017453292519943295*b.longitude);b=Math.sin(.017453292519943295*d);var m=Math.cos(.017453292519943295*d),n=Math.sin(.2617993877991494*c),q=Math.cos(.2617993877991494*c),u=[k*g,k*l,f];f=[-f*g,-f*l,k];l=[l,-g,0];k=-15*pa(a);a=ha(k,u);u=ha(k,f);l=ha(k,l);b=[m*q,m*n,b];n=b[0]*a[0]+b[1]*a[1]+b[2]*a[2];m=b[0]*u[0]+b[1]*u[1]+b[2]*u[2];u=b[0]*l[0]+b[1]*l[1]+b[2]*l[2];q=Math.sqrt(m*m+u*u);0m&&(m+=360)):m=0;n=57.29577951308232*Math.atan2(q,n);q=d;if(e&&(d=n,e=ra(e,90-n),n-=e,0l;++l)e.push((b[l]-d*a[l])/u*c+a[l]*q);q=Math.sqrt(e[0]*e[0]+e[1]*e[1]);0c&&(c+=24)):c=0;q=57.29577951308232*Math.atan2(e[2],q)}return new zb(m,90-n,c,q)}function ia(a){if(!(a instanceof
+Ab))throw"Not an instance of the Observer class: "+a;r(a.latitude);r(a.longitude);r(a.height);if(-90>a.latitude||90d&&(d+=360));return new Db(a,f,b,57.29577951308232*Math.atan2(b,c),d)}function sa(a,b,c){void 0===Ka&&(Ka=.017453292519943295*Ca(y(ab)).mobl,Eb=Math.cos(Ka),Fb=Math.sin(Ka));r(a);r(b);r(c);return Cb(a,b,c,Eb,Fb)}function X(a){a=y(a);var b=S(a),c=b.distance_au*
+Math.cos(b.geo_eclip_lat);b=[c*Math.cos(b.geo_eclip_lon),c*Math.sin(b.geo_eclip_lon),b.distance_au*Math.sin(b.geo_eclip_lat)];var d=.017453292519943295*na(a);c=Math.cos(d);d=Math.sin(d);b=Ha(a.tt,[b[0],b[1]*c-b[2]*d,b[1]*d+b[2]*c],0);return new B(b[0],b[1],b[2],a)}function ba(a,b){var c=1,d=0;a=$jscomp.makeIterator(a);for(var e=a.next();!e.done;e=a.next()){var f=0;e=$jscomp.makeIterator(e.value);for(var k=e.next();!k.done;k=e.next()){var l=$jscomp.makeIterator(k.value);k=l.next().value;var g=l.next().value;
l=l.next().value;f+=k*Math.cos(g+b*l)}d+=c*f;c*=b}return d}function bb(a,b){var c=1,d=0,e=0,f=0;a=$jscomp.makeIterator(a);for(var k=a.next();!k.done;k=a.next()){var l=0,g=0;k=$jscomp.makeIterator(k.value);for(var m=k.next();!m.done;m=k.next()){var n=$jscomp.makeIterator(m.value);m=n.next().value;var q=n.next().value;n=n.next().value;q+=b*n;l+=m*n*Math.sin(q);0a?0:a>=b?b-1:a}function eb(a){var b=$jscomp.makeIterator(a);a=b.next().value;var c=$jscomp.makeIterator(b.next().value);var d=c.next().value;var e=c.next().value;c=c.next().value;var f=$jscomp.makeIterator(b.next().value);b=f.next().value;var k=f.next().value;f=f.next().value;d=new Na(a,new C(d,e,c),new C(b,k,f));a=new Pa(d.tt);
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-[];f[146]=c[146];for(d=145;0a?0:a>=b?b-1:a}function eb(a){var b=$jscomp.makeIterator(a);a=b.next().value;var c=$jscomp.makeIterator(b.next().value);var d=c.next().value;var e=c.next().value;c=c.next().value;var f=$jscomp.makeIterator(b.next().value);b=f.next().value;var k=f.next().value;f=f.next().value;d=new Na(a,new C(d,e,c),new C(b,k,f));a=new Pa(d.tt);
+e=d.r.add(a.Sun.r);c=d.v.add(a.Sun.v);b=a.Acceleration(e);d=new Hb(d.tt,e,c,b);return new Ib(a,d)}function Kb(a,b,c){a=eb(a);for(var d=Math.ceil((b-a.grav.tt)/c),e=0;eca[40][0])a=null;else{a=Jb((a-c)/36500,40);if(!fb[a]){c=fb[a]=[];c[0]=eb(ca[a]).grav;c[146]=eb(ca[a+1]).grav;var d,e=c[0].tt;for(d=1;146>d;++d)c[d]=db(e+=250,c[d-1]).grav;e=c[146].tt;var f=
+[];f[146]=c[146];for(d=145;0l;++l){e=ua(a,k);c?d=N(F.Earth,k):d||(d=N(F.Earth,b));e=new B(e.x-d.x,e.y-d.y,e.z-d.z,b);var g=b.AddDays(-e.Length()/173.1446326846693);f=Math.abs(g.tt-k.tt);if(1E-9>f)return e;k=g}throw"Light-travel time solver did not converge: dt="+f;}function yc(a,b,c,d,e){var f=(e+c)/2-d;c=(e-c)/2;if(0==f){if(0==c)return null;d=-d/c;if(-1>d||1=d)return null;e=Math.sqrt(d);d=(-c+e)/(2*f);e=(-c-e)/(2*f);if(-1<=d&&1>=d){if(-1<=e&&1>=e)return null}else if(-1<=e&&1>=e)d=e;else return null}return{x:d,t:a+d*b,df_dt:(2*f*d+c)/b}}function E(a,b,c,d){var e=r(d&&d.dt_tolerance_seconds||1);e=Math.abs(e/86400);var f=d&&d.init_f1||a(b),k=d&&d.init_f2||a(c),l=NaN,g=0;d=d&&d.iter_limit||20;for(var m=!0;;){if(++g>d)throw"Excessive iteration in Search()";var n=new P(b.ut+.5*(c.ut-b.ut)),q=n.ut-b.ut;if(Math.abs(q)(q.ut-b.ut)*(q.ut-c.ut)&&0>(w.ut-b.ut)*(w.ut-c.ut))){u=a(q);var z=a(w);if(0>u&&0<=z){f=u;k=z;b=q;c=w;l=H;m=!1;continue}}}}if(0>f&&0<=l)c=n,k=l;else if(0>l&&0<=k)b=n,f=l;else return null}}function va(a){for(;-180>=a;)a+=360;for(;180b;)b+=360;for(;360<=b;)b-=360;return b}function ka(a,b){if("Earth"==a)throw"The Earth does not have an angle as seen from itself.";var c=W("Sun",b,!0);a=W(a,b,!0);return O(c,a)}function ea(a,b){if("Sun"===a)throw"Cannot calculate heliocentric longitude of the Sun.";a=ua(a,b);return sa(a.x,a.y,a.z).elon}
-function Qa(a,b){if("Earth"===a)throw"The illumination of the Earth is not defined.";var c=y(b),d=N(F.Earth,c);if("Sun"===a){var e=new B(-d.x,-d.y,-d.z,c);b=new B(0,0,0,c);d=0}else"Moon"===a?(e=X(c),b=new B(d.x+e.x,d.y+e.y,d.z+e.z,c)):(b=ua(a,b),e=new B(b.x-d.x,b.y-d.y,b.z-d.z,c)),d=O(e,b);var f=e.Length(),k=b.Length();if("Sun"===a)a=zc+5*Math.log10(f);else if("Moon"===a){a=.017453292519943295*d;var l=a*a;a=-12.717+1.49*Math.abs(a)+.0431*l*l;a+=5*Math.log10(f/.002573570052980638*k)}else if("Saturn"===
+b).Length()}function W(a,b,c){x(c);b=y(b);if("Moon"===a)return X(b);if("Earth"===a)return new B(0,0,0,b);for(var d=null,e,f=0,k=b,l=0;10>l;++l){e=ua(a,k);c?d=N(F.Earth,k):d||(d=N(F.Earth,b));e=new B(e.x-d.x,e.y-d.y,e.z-d.z,b);var g=b.AddDays(-e.Length()/173.1446326846693);f=Math.abs(g.tt-k.tt);if(1E-9>f)return e;k=g}throw"Light-travel time solver did not converge: dt="+f;}function xc(a,b,c,d,e){var f=(e+c)/2-d;c=(e-c)/2;if(0==f){if(0==c)return null;d=-d/c;if(-1>d||1=d)return null;e=Math.sqrt(d);d=(-c+e)/(2*f);e=(-c-e)/(2*f);if(-1<=d&&1>=d){if(-1<=e&&1>=e)return null}else if(-1<=e&&1>=e)d=e;else return null}return{x:d,t:a+d*b,df_dt:(2*f*d+c)/b}}function E(a,b,c,d){var e=r(d&&d.dt_tolerance_seconds||1);e=Math.abs(e/86400);var f=d&&d.init_f1||a(b),k=d&&d.init_f2||a(c),l=NaN,g=0;d=d&&d.iter_limit||20;for(var m=!0;;){if(++g>d)throw"Excessive iteration in Search()";var n=new P(b.ut+.5*(c.ut-b.ut)),q=n.ut-b.ut;if(Math.abs(q)(q.ut-b.ut)*(q.ut-c.ut)&&0>(w.ut-b.ut)*(w.ut-c.ut))){u=a(q);var z=a(w);if(0>u&&0<=z){f=u;k=z;b=q;c=w;l=H;m=!1;continue}}}}if(0>f&&0<=l)c=n,k=l;else if(0>l&&0<=k)b=n,f=l;else return null}}function va(a){for(;-180>=a;)a+=360;for(;180b;)b+=360;for(;360<=b;)b-=360;return b}function ja(a,b){if("Earth"==a)throw"The Earth does not have an angle as seen from itself.";var c=W("Sun",b,!0);a=W(a,b,!0);return O(c,a)}function ea(a,b){if("Sun"===a)throw"Cannot calculate heliocentric longitude of the Sun.";a=ua(a,b);return sa(a.x,a.y,a.z).elon}
+function Qa(a,b){if("Earth"===a)throw"The illumination of the Earth is not defined.";var c=y(b),d=N(F.Earth,c);if("Sun"===a){var e=new B(-d.x,-d.y,-d.z,c);b=new B(0,0,0,c);d=0}else"Moon"===a?(e=X(c),b=new B(d.x+e.x,d.y+e.y,d.z+e.z,c)):(b=ua(a,b),e=new B(b.x-d.x,b.y-d.y,b.z-d.z,c)),d=O(e,b);var f=e.Length(),k=b.Length();if("Sun"===a)a=yc+5*Math.log10(f);else if("Moon"===a){a=.017453292519943295*d;var l=a*a;a=-12.717+1.49*Math.abs(a)+.0431*l*l;a+=5*Math.log10(f/.002573570052980638*k)}else if("Saturn"===
a){a=d;var g=sa(e.x,e.y,e.z);l=.017453292519943295*g.elat;g=Math.asin(Math.sin(l)*Math.cos(.4897393881096089)-Math.cos(l)*Math.sin(.4897393881096089)*Math.sin(.017453292519943295*g.elon-.017453292519943295*(169.51+3.82E-5*c.tt)));l=Math.sin(Math.abs(g));a=-9+.044*a+l*(-2.6+1.2*l)+5*Math.log10(k*f);g*=57.29577951308232}else{var m=l=0,n=0;switch(a){case "Mercury":a=-.6;l=4.98;m=-4.88;n=3.02;break;case "Venus":163.6>d?(a=-4.47,l=1.03,m=.57,n=.13):(a=.98,l=-1.02);break;case "Mars":a=-1.52;l=1.6;break;
-case "Jupiter":a=-9.4;l=.5;break;case "Uranus":a=-7.19;l=.25;break;case "Neptune":a=-6.87;break;case "Pluto":a=-1;l=4;break;default:throw"VisualMagnitude: unsupported body "+a;}var q=d/100;a=a+q*(l+q*(m+q*n))+5*Math.log10(k*f)}return new Nb(c,a,d,k,f,e,b,g)}function wa(a){if("Earth"===a)throw"The Earth does not have a synodic period as seen from itself.";if("Moon"===a)return 29.530588;var b=Y[a];if(!b)throw"Not a valid planet name: "+a;a=Y.Earth.OrbitalPeriod;return Math.abs(a/(a/b.OrbitalPeriod-
-1))}function la(a,b,c){function d(m){var n=ea(a,m);m=ea("Earth",m);return va(f*(m-n)-b)}r(b);var e=Y[a];if(!e)throw"Cannot search relative longitude because body is not a planet: "+a;if("Earth"===a)throw"Cannot search relative longitude for the Earth (it is always 0)";var f=e.OrbitalPeriod>Y.Earth.OrbitalPeriod?1:-1;e=wa(a);c=y(c);var k=d(c);0l;++l){var g=-k/360*e;c=c.AddDays(g);if(1>86400*Math.abs(g))return c;g=k;k=d(c);30>Math.abs(g)&&g!==k&&(g/=g-k,.5g&&(e*=g))}throw"Relative longitude search failed to converge for "+
-a+" near "+c.toString()+" (error_angle = "+k+").";}function hb(a){return gb("Moon",a)}function xa(a,b,c){function d(k){k=hb(k);return va(k-a)}r(a);r(c);b=y(b);var e=d(b);0c)return null;c=Math.min(c,f+1.5);e=b.AddDays(e);b=b.AddDays(c);return E(d,e,b)}function Ob(a){var b=hb(a);b=(Math.floor(b/90)+1)%4;a=xa(90*b,a,10);if(!a)throw"Cannot find moon quarter";return new Pb(b,a)}function ya(a,b,c,d){ja(b);d=y(d);var e=0;if("Earth"===a)throw"Cannot search for hour angle of the Earth.";
-r(c);if(0>c||24<=c)throw"Invalid hour angle "+c;for(;;){++e;var f=qa(d),k=Ja(a,d,b,!0,!0);f=(c+k.ra-b.longitude/15-f)%24;1===e?0>f&&(f+=24):-12>f?f+=24:123600*Math.abs(f))return a=Ia(d,b,k.ra,k.dec,"normal"),new Qb(d,a);d=d.AddDays(f/24*.9972695717592592)}}function Rb(a,b){b=y(b);var c=gb(a,b);if(180Y.Earth.OrbitalPeriod?1:-1;e=wa(a);c=y(c);var k=d(c);0l;++l){var g=-k/360*e;c=c.AddDays(g);if(1>86400*Math.abs(g))return c;g=k;k=d(c);30>Math.abs(g)&&g!==k&&(g/=g-k,.5g&&(e*=g))}throw"Relative longitude search failed to converge for "+
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-b=y(b);for(var d=0;2>=++d;){var e=ea(a,b),f=ea("Earth",b),k=va(e-f),l=e=f=void 0;-10<=k&&10>k?(l=0,f=10,e=30):30<=k||-30>k?(l=0,f=-30,e=-10):0<=k?(l=-wa(a)/4,f=10,e=30):(l=-wa(a)/4,f=-30,e=-10);k=b.AddDays(l);f=la(a,f,k);e=la(a,e,f);k=c(f);if(0<=k)throw"SearchPeakMagnitude: internal error: m1 = "+k;l=c(e);if(0>=l)throw"SearchPeakMagnitude: internal error: m2 = "+l;k=E(c,f,e,{init_f1:k,init_f2:l,dt_tolerance_seconds:10});if(!k)throw"SearchPeakMagnitude: failed search iter "+d+" (t1="+f.toString()+
-", t2="+e.toString()+")";if(k.tt>=b.tt)return Qa(a,k);b=e.AddDays(1)}throw"SearchPeakMagnitude: failed to find event after 2 tries.";};var za=function(a,b,c){this.time=a;this.kind=b;this.dist_au=c;this.dist_km=1.4959787069098932E8*c};h.Apsis=za;h.SearchLunarApsis=Tb;h.NextLunarApsis=function(a){var b=Tb(a.time.AddDays(11));if(1!==b.kind+a.kind)throw"NextLunarApsis INTERNAL ERROR: did not find alternating apogee/perigee: prev="+a.kind+" @ "+a.time.toString()+", next="+b.kind+" @ "+b.time.toString();
-return b};h.SearchPlanetApsis=Vb;h.NextPlanetApsis=function(a,b){if(0!==b.kind&&1!==b.kind)throw"Invalid apsis kind: "+b.kind;var c=b.time.AddDays(.25*Y[a].OrbitalPeriod);a=Vb(a,c);if(1!==a.kind+b.kind)throw"Internal error: previous apsis was "+b.kind+", but found "+a.kind+" for next apsis.";return a};h.InverseRotation=ma;h.CombineRotation=na;h.IdentityMatrix=function(){return new K([[1,0,0],[0,1,0],[0,0,1]])};h.Pivot=function(a,b,c){if(0!==b&&1!==b&&2!==b)throw"Invalid axis "+b+". Must be [0, 1, 2].";
-var d=.017453292519943295*r(c);c=Math.cos(d);d=Math.sin(d);var e=(b+1)%3,f=(b+2)%3,k=[[0,0,0],[0,0,0],[0,0,0]];k[e][e]=c*a.rot[e][e]-d*a.rot[e][f];k[e][f]=d*a.rot[e][e]+c*a.rot[e][f];k[e][b]=a.rot[e][b];k[f][e]=c*a.rot[f][e]-d*a.rot[f][f];k[f][f]=d*a.rot[f][e]+c*a.rot[f][f];k[f][b]=a.rot[f][b];k[b][e]=c*a.rot[b][e]-d*a.rot[b][f];k[b][f]=d*a.rot[b][e]+c*a.rot[b][f];k[b][b]=a.rot[b][b];return new K(k)};h.VectorFromSphere=ib;h.VectorFromEquator=Wb;h.EquatorFromVector=Xb;h.SphereFromVector=jb;h.HorizonFromVector=
-function(a,b){a=jb(a);a.lon=Yb(a.lon);a.lat+=ra(b,a.lat);return a};h.VectorFromHorizon=function(a,b,c){var d=Yb(a.lon);c=a.lat+Zb(c,a.lat);a=new Ra(c,d,a.dist);return ib(a,b)};h.Refraction=ra;h.InverseRefraction=Zb;h.RotateVector=Aa;h.Rotation_EQJ_ECL=$b;h.Rotation_ECL_EQJ=function(){return new K([[1,0,0],[0,.9174821430670688,.3977769691083922],[0,-.3977769691083922,.9174821430670688]])};h.Rotation_EQJ_EQD=kb;h.Rotation_EQD_EQJ=lb;h.Rotation_EQD_HOR=mb;h.Rotation_HOR_EQD=ac;h.Rotation_HOR_EQJ=bc;
-h.Rotation_EQJ_HOR=function(a,b){a=bc(a,b);return ma(a)};h.Rotation_EQD_ECL=cc;h.Rotation_ECL_EQD=dc;h.Rotation_ECL_HOR=ec;h.Rotation_HOR_ECL=function(a,b){a=ec(a,b);return ma(a)};var Hc=[["And","Andromeda"],["Ant","Antila"],["Aps","Apus"],["Aql","Aquila"],["Aqr","Aquarius"],["Ara","Ara"],["Ari","Aries"],["Aur","Auriga"],["Boo","Bootes"],["Cae","Caelum"],["Cam","Camelopardis"],["Cap","Capricornus"],["Car","Carina"],["Cas","Cassiopeia"],["Cen","Centaurus"],["Cep","Cepheus"],["Cet","Cetus"],["Cha",
-"Chamaeleon"],["Cir","Circinus"],["CMa","Canis Major"],["CMi","Canis Minor"],["Cnc","Cancer"],["Col","Columba"],["Com","Coma Berenices"],["CrA","Corona Australis"],["CrB","Corona Borealis"],["Crt","Crater"],["Cru","Crux"],["Crv","Corvus"],["CVn","Canes Venatici"],["Cyg","Cygnus"],["Del","Delphinus"],["Dor","Dorado"],["Dra","Draco"],["Equ","Equuleus"],["Eri","Eridanus"],["For","Fornax"],["Gem","Gemini"],["Gru","Grus"],["Her","Hercules"],["Hor","Horologium"],["Hya","Hydra"],["Hyi","Hydrus"],["Ind",
-"Indus"],["Lac","Lacerta"],["Leo","Leo"],["Lep","Lepus"],["Lib","Libra"],["LMi","Leo Minor"],["Lup","Lupus"],["Lyn","Lynx"],["Lyr","Lyra"],["Men","Mensa"],["Mic","Microscopium"],["Mon","Monoceros"],["Mus","Musca"],["Nor","Norma"],["Oct","Octans"],["Oph","Ophiuchus"],["Ori","Orion"],["Pav","Pavo"],["Peg","Pegasus"],["Per","Perseus"],["Phe","Phoenix"],["Pic","Pictor"],["PsA","Pisces Austrinus"],["Psc","Pisces"],["Pup","Puppis"],["Pyx","Pyxis"],["Ret","Reticulum"],["Scl","Sculptor"],["Sco","Scorpius"],
-["Sct","Scutum"],["Ser","Serpens"],["Sex","Sextans"],["Sge","Sagitta"],["Sgr","Sagittarius"],["Tau","Taurus"],["Tel","Telescopium"],["TrA","Triangulum Australe"],["Tri","Triangulum"],["Tuc","Tucana"],["UMa","Ursa Major"],["UMi","Ursa Minor"],["Vel","Vela"],["Vir","Virgo"],["Vol","Volans"],["Vul","Vulpecula"]],Ic=[[83,0,8640,2112],[83,2880,5220,2076],[83,7560,8280,2068],[83,6480,7560,2064],[15,0,2880,2040],[10,3300,3840,1968],[15,0,1800,1920],[10,3840,5220,1920],[83,6300,6480,1920],[33,7260,7560,1920],
-[15,0,1263,1848],[10,4140,4890,1848],[83,5952,6300,1800],[15,7260,7440,1800],[10,2868,3300,1764],[33,3300,4080,1764],[83,4680,5952,1680],[13,1116,1230,1632],[33,7350,7440,1608],[33,4080,4320,1596],[15,0,120,1584],[83,5040,5640,1584],[15,8490,8640,1584],[33,4320,4860,1536],[33,4860,5190,1512],[15,8340,8490,1512],[10,2196,2520,1488],[33,7200,7350,1476],[15,7393.2,7416,1462],[10,2520,2868,1440],[82,2868,3030,1440],[33,7116,7200,1428],[15,7200,7393.2,1428],[15,8232,8340,1418],[13,0,876,1404],[33,6990,
-7116,1392],[13,612,687,1380],[13,876,1116,1368],[10,1116,1140,1368],[15,8034,8232,1350],[10,1800,2196,1344],[82,5052,5190,1332],[33,5190,6990,1332],[10,1140,1200,1320],[15,7968,8034,1320],[15,7416,7908,1316],[13,0,612,1296],[50,2196,2340,1296],[82,4350,4860,1272],[33,5490,5670,1272],[15,7908,7968,1266],[10,1200,1800,1260],[13,8232,8400,1260],[33,5670,6120,1236],[62,735,906,1212],[33,6120,6564,1212],[13,0,492,1200],[62,492,600,1200],[50,2340,2448,1200],[13,8400,8640,1200],[82,4860,5052,1164],[13,0,
-402,1152],[13,8490,8640,1152],[39,6543,6564,1140],[33,6564,6870,1140],[30,6870,6900,1140],[62,600,735,1128],[82,3030,3300,1128],[13,60,312,1104],[82,4320,4350,1080],[50,2448,2652,1068],[30,7887,7908,1056],[30,7875,7887,1050],[30,6900,6984,1044],[82,3300,3660,1008],[82,3660,3882,960],[8,5556,5670,960],[39,5670,5880,960],[50,3330,3450,954],[0,0,906,882],[62,906,924,882],[51,6969,6984,876],[62,1620,1689,864],[30,7824,7875,864],[44,7875,7920,864],[7,2352,2652,852],[50,2652,2790,852],[0,0,720,840],[44,
-7920,8214,840],[44,8214,8232,828],[0,8232,8460,828],[62,924,978,816],[82,3882,3960,816],[29,4320,4440,816],[50,2790,3330,804],[48,3330,3558,804],[0,258,507,792],[8,5466,5556,792],[0,8460,8550,770],[29,4440,4770,768],[0,8550,8640,752],[29,5025,5052,738],[80,870,978,736],[62,978,1620,736],[7,1620,1710,720],[51,6543,6969,720],[82,3960,4320,696],[30,7080,7530,696],[7,1710,2118,684],[48,3558,3780,684],[29,4770,5025,684],[0,0,24,672],[80,507,600,672],[7,2118,2352,672],[37,2838,2880,672],[30,7530,7824,672],
-[30,6933,7080,660],[80,690,870,654],[25,5820,5880,648],[8,5430,5466,624],[25,5466,5820,624],[51,6612,6792,624],[48,3870,3960,612],[51,6792,6933,612],[80,600,690,600],[66,258,306,570],[48,3780,3870,564],[87,7650,7710,564],[77,2052,2118,548],[0,24,51,528],[73,5730,5772,528],[37,2118,2238,516],[87,7140,7290,510],[87,6792,6930,506],[0,51,306,504],[87,7290,7404,492],[37,2811,2838,480],[87,7404,7650,468],[87,6930,7140,460],[6,1182,1212,456],[75,6792,6840,444],[59,2052,2076,432],[37,2238,2271,420],[75,6840,
-7140,388],[77,1788,1920,384],[39,5730,5790,384],[75,7140,7290,378],[77,1662,1788,372],[77,1920,2016,372],[23,4620,4860,360],[39,6210,6570,344],[23,4272,4620,336],[37,2700,2811,324],[39,6030,6210,308],[61,0,51,300],[77,2016,2076,300],[37,2520,2700,300],[61,7602,7680,300],[37,2271,2496,288],[39,6570,6792,288],[31,7515,7578,284],[61,7578,7602,284],[45,4146,4272,264],[59,2247,2271,240],[37,2496,2520,240],[21,2811,2853,240],[61,8580,8640,240],[6,600,1182,238],[31,7251,7308,204],[8,4860,5430,192],[61,8190,
-8580,180],[21,2853,3330,168],[45,3330,3870,168],[58,6570,6718.4,150],[3,6718.4,6792,150],[31,7500,7515,144],[20,2520,2526,132],[73,6570,6633,108],[39,5790,6030,96],[58,6570,6633,72],[61,7728,7800,66],[66,0,720,48],[73,6690,6792,48],[31,7308,7500,48],[34,7500,7680,48],[61,7680,7728,48],[61,7920,8190,48],[61,7800,7920,42],[20,2526,2592,36],[77,1290,1662,0],[59,1662,1680,0],[20,2592,2910,0],[85,5280,5430,0],[58,6420,6570,0],[16,954,1182,-42],[77,1182,1290,-42],[73,5430,5856,-78],[59,1680,1830,-96],[59,
-2100,2247,-96],[73,6420,6468,-96],[73,6570,6690,-96],[3,6690,6792,-96],[66,8190,8580,-96],[45,3870,4146,-144],[85,4146,4260,-144],[66,0,120,-168],[66,8580,8640,-168],[85,5130,5280,-192],[58,5730,5856,-192],[3,7200,7392,-216],[4,7680,7872,-216],[58,6180,6468,-240],[54,2100,2910,-264],[35,1770,1830,-264],[59,1830,2100,-264],[41,2910,3012,-264],[74,3450,3870,-264],[85,4260,4620,-264],[58,6330,6360,-280],[3,6792,7200,-288.8],[35,1740,1770,-348],[4,7392,7680,-360],[73,6180,6570,-384],[72,6570,6792,-384],
-[41,3012,3090,-408],[58,5856,5895,-438],[41,3090,3270,-456],[26,3870,3900,-456],[71,5856,5895,-462],[47,5640,5730,-480],[28,4530,4620,-528],[85,4620,5130,-528],[41,3270,3510,-576],[16,600,954,-585.2],[35,954,1350,-585.2],[26,3900,4260,-588],[28,4260,4530,-588],[47,5130,5370,-588],[58,5856,6030,-590],[16,0,600,-612],[11,7680,7872,-612],[4,7872,8580,-612],[16,8580,8640,-612],[41,3510,3690,-636],[35,1692,1740,-654],[46,1740,2202,-654],[11,7200,7680,-672],[41,3690,3810,-700],[41,4530,5370,-708],[47,5370,
-5640,-708],[71,5640,5760,-708],[35,1650,1692,-720],[58,6030,6336,-720],[76,6336,6420,-720],[41,3810,3900,-748],[19,2202,2652,-792],[41,4410,4530,-792],[41,3900,4410,-840],[36,1260,1350,-864],[68,3012,3372,-882],[35,1536,1650,-888],[76,6420,6900,-888],[65,7680,8280,-888],[70,8280,8400,-888],[36,1080,1260,-950],[1,3372,3960,-954],[70,0,600,-960],[36,600,1080,-960],[35,1392,1536,-960],[70,8400,8640,-960],[14,5100,5370,-1008],[49,5640,5760,-1008],[71,5760,5911.5,-1008],[9,1740,1800,-1032],[22,1800,2370,
--1032],[67,2880,3012,-1032],[35,1230,1392,-1056],[71,5911.5,6420,-1092],[24,6420,6900,-1092],[76,6900,7320,-1092],[53,7320,7680,-1092],[35,1080,1230,-1104],[9,1620,1740,-1116],[49,5520,5640,-1152],[63,0,840,-1156],[35,960,1080,-1176],[40,1470,1536,-1176],[9,1536,1620,-1176],[38,7680,7920,-1200],[67,2160,2880,-1218],[84,2880,2940,-1218],[35,870,960,-1224],[40,1380,1470,-1224],[63,0,660,-1236],[12,2160,2220,-1260],[84,2940,3042,-1272],[40,1260,1380,-1276],[32,1380,1440,-1276],[63,0,570,-1284],[35,780,
-870,-1296],[64,1620,1800,-1296],[49,5418,5520,-1296],[84,3042,3180,-1308],[12,2220,2340,-1320],[14,4260,4620,-1320],[49,5100,5418,-1320],[56,5418,5520,-1320],[32,1440,1560,-1356],[84,3180,3960,-1356],[14,3960,4050,-1356],[5,6300,6480,-1368],[78,6480,7320,-1368],[38,7920,8400,-1368],[40,1152,1260,-1380],[64,1800,1980,-1380],[12,2340,2460,-1392],[63,0,480,-1404],[35,480,780,-1404],[63,8400,8640,-1404],[32,1560,1650,-1416],[56,5520,5911.5,-1440],[43,7320,7680,-1440],[64,1980,2160,-1464],[18,5460,5520,
--1464],[5,5911.5,5970,-1464],[18,5370,5460,-1526],[5,5970,6030,-1526],[64,2160,2460,-1536],[12,2460,3252,-1536],[14,4050,4260,-1536],[27,4260,4620,-1536],[14,4620,5232,-1536],[18,4860,4920,-1560],[5,6030,6060,-1560],[40,780,1152,-1620],[69,1152,1650,-1620],[18,5310,5370,-1620],[5,6060,6300,-1620],[60,6300,6480,-1620],[81,7920,8400,-1620],[32,1650,2370,-1680],[18,4920,5310,-1680],[79,5310,6120,-1680],[81,0,480,-1800],[42,1260,1650,-1800],[86,2370,3252,-1800],[12,3252,4050,-1800],[55,4050,4920,-1800],
-[60,6480,7680,-1800],[43,7680,8400,-1800],[81,8400,8640,-1800],[81,270,480,-1824],[42,0,1260,-1980],[17,2760,4920,-1980],[2,4920,6480,-1980],[52,1260,2760,-2040],[57,0,8640,-2160]],qb,rb,uc=function(a,b,c,d){this.symbol=a;this.name=b;this.ra1875=c;this.dec1875=d};h.ConstellationInfo=uc;h.Constellation=function(a,b){r(a);r(b);if(-90>b||90a&&(a+=24);qb||(qb=kb(new P(-45655.74141261017)),rb=new P(0));var c=new B(0,0,0,rb);a=new ha(a,b,1,
-c);a=Wb(a,rb);a=Aa(qb,a);a=Xb(a);b=10/240;c=b/15;for(var d=$jscomp.makeIterator(Ic),e=d.next();!e.done;e=d.next()){e=e.value;var f=e[1]*c,k=e[2]*c;if(e[3]*b<=a.dec&&f<=a.ra&&a.ra=m&&0=d.ut+e)return null;q=m.time;m=f(m.time);n=f(u.time)}};var Pb=function(a,b){this.time=a;this.hor=b};h.HourAngleEvent=Pb;h.SearchHourAngle=ya;var rc=function(a,b,c,d){this.mar_equinox=a;this.jun_solstice=b;this.sep_equinox=c;this.dec_solstice=d};h.SeasonInfo=rc;h.Seasons=function(a){function b(k,l,g){l=new Date(Date.UTC(a,l-1,g));k=Lb(k,l,4);if(!k)throw"Cannot find season change near "+
+l.toISOString();return k}a instanceof Date&&Number.isFinite(a.getTime())&&(a=a.getUTCFullYear());if(!Number.isSafeInteger(a))throw"Cannot calculate seasons because year argument "+a+" is neither a Date nor a safe integer.";var c=b(0,3,19),d=b(90,6,19),e=b(180,9,21),f=b(270,12,20);return new rc(c,d,e,f)};var Rb=function(a,b,c,d){this.time=a;this.visibility=b;this.elongation=c;this.ecliptic_separation=d};h.ElongationEvent=Rb;h.Elongation=Qb;h.SearchMaxElongation=function(a,b){function c(m){var n=m.AddDays(-.005);
+m=m.AddDays(.005);n=ja(a,n);m=ja(a,m);return(n-m)/.01}b=y(b);var d={Mercury:{s1:50,s2:85},Venus:{s1:40,s2:50}}[a];if(!d)throw"SearchMaxElongation works for Mercury and Venus only.";for(var e=0;2>=++e;){var f=ea(a,b),k=ea("Earth",b),l=va(f-k),g=f=k=void 0;l>=-d.s1&&l<+d.s1?(g=0,k=+d.s1,f=+d.s2):l>=+d.s2||l<-d.s2?(g=0,k=-d.s2,f=-d.s1):0<=l?(g=-wa(a)/4,k=+d.s1,f=+d.s2):(g=-wa(a)/4,k=-d.s2,f=-d.s1);l=b.AddDays(g);k=ka(a,k,l);f=ka(a,f,k);l=c(k);if(0<=l)throw"SearchMaxElongation: internal error: m1 = "+
+l;g=c(f);if(0>=g)throw"SearchMaxElongation: internal error: m2 = "+g;l=E(c,k,f,{init_f1:l,init_f2:g,dt_tolerance_seconds:10});if(!l)throw"SearchMaxElongation: failed search iter "+e+" (t1="+k.toString()+", t2="+f.toString()+")";if(l.tt>=b.tt)return Qb(a,l);b=f.AddDays(1)}throw"SearchMaxElongation: failed to find event after 2 tries.";};h.SearchPeakMagnitude=function(a,b){function c(g){var m=g.AddDays(-.005);g=g.AddDays(.005);m=Qa(a,m).mag;return(Qa(a,g).mag-m)/.01}if("Venus"!==a)throw"SearchPeakMagnitude currently works for Venus only.";
+b=y(b);for(var d=0;2>=++d;){var e=ea(a,b),f=ea("Earth",b),k=va(e-f),l=e=f=void 0;-10<=k&&10>k?(l=0,f=10,e=30):30<=k||-30>k?(l=0,f=-30,e=-10):0<=k?(l=-wa(a)/4,f=10,e=30):(l=-wa(a)/4,f=-30,e=-10);k=b.AddDays(l);f=ka(a,f,k);e=ka(a,e,f);k=c(f);if(0<=k)throw"SearchPeakMagnitude: internal error: m1 = "+k;l=c(e);if(0>=l)throw"SearchPeakMagnitude: internal error: m2 = "+l;k=E(c,f,e,{init_f1:k,init_f2:l,dt_tolerance_seconds:10});if(!k)throw"SearchPeakMagnitude: failed search iter "+d+" (t1="+f.toString()+
+", t2="+e.toString()+")";if(k.tt>=b.tt)return Qa(a,k);b=e.AddDays(1)}throw"SearchPeakMagnitude: failed to find event after 2 tries.";};var za=function(a,b,c){this.time=a;this.kind=b;this.dist_au=c;this.dist_km=1.4959787069098932E8*c};h.Apsis=za;h.SearchLunarApsis=Sb;h.NextLunarApsis=function(a){var b=Sb(a.time.AddDays(11));if(1!==b.kind+a.kind)throw"NextLunarApsis INTERNAL ERROR: did not find alternating apogee/perigee: prev="+a.kind+" @ "+a.time.toString()+", next="+b.kind+" @ "+b.time.toString();
+return b};h.SearchPlanetApsis=Ub;h.NextPlanetApsis=function(a,b){if(0!==b.kind&&1!==b.kind)throw"Invalid apsis kind: "+b.kind;var c=b.time.AddDays(.25*Y[a].OrbitalPeriod);a=Ub(a,c);if(1!==a.kind+b.kind)throw"Internal error: previous apsis was "+b.kind+", but found "+a.kind+" for next apsis.";return a};h.InverseRotation=la;h.CombineRotation=ma;h.IdentityMatrix=function(){return new K([[1,0,0],[0,1,0],[0,0,1]])};h.Pivot=function(a,b,c){if(0!==b&&1!==b&&2!==b)throw"Invalid axis "+b+". Must be [0, 1, 2].";
+var d=.017453292519943295*r(c);c=Math.cos(d);d=Math.sin(d);var e=(b+1)%3,f=(b+2)%3,k=[[0,0,0],[0,0,0],[0,0,0]];k[e][e]=c*a.rot[e][e]-d*a.rot[e][f];k[e][f]=d*a.rot[e][e]+c*a.rot[e][f];k[e][b]=a.rot[e][b];k[f][e]=c*a.rot[f][e]-d*a.rot[f][f];k[f][f]=d*a.rot[f][e]+c*a.rot[f][f];k[f][b]=a.rot[f][b];k[b][e]=c*a.rot[b][e]-d*a.rot[b][f];k[b][f]=d*a.rot[b][e]+c*a.rot[b][f];k[b][b]=a.rot[b][b];return new K(k)};h.VectorFromSphere=ib;h.EquatorFromVector=Vb;h.SphereFromVector=jb;h.HorizonFromVector=function(a,
+b){a=jb(a);a.lon=Wb(a.lon);a.lat+=ra(b,a.lat);return a};h.VectorFromHorizon=function(a,b,c){var d=Wb(a.lon);c=a.lat+Xb(c,a.lat);a=new Ra(c,d,a.dist);return ib(a,b)};h.Refraction=ra;h.InverseRefraction=Xb;h.RotateVector=Aa;h.Rotation_EQJ_ECL=Yb;h.Rotation_ECL_EQJ=function(){return new K([[1,0,0],[0,.9174821430670688,.3977769691083922],[0,-.3977769691083922,.9174821430670688]])};h.Rotation_EQJ_EQD=kb;h.Rotation_EQD_EQJ=lb;h.Rotation_EQD_HOR=mb;h.Rotation_HOR_EQD=Zb;h.Rotation_HOR_EQJ=$b;h.Rotation_EQJ_HOR=
+function(a,b){a=$b(a,b);return la(a)};h.Rotation_EQD_ECL=ac;h.Rotation_ECL_EQD=bc;h.Rotation_ECL_HOR=cc;h.Rotation_HOR_ECL=function(a,b){a=cc(a,b);return la(a)};var Gc=[["And","Andromeda"],["Ant","Antila"],["Aps","Apus"],["Aql","Aquila"],["Aqr","Aquarius"],["Ara","Ara"],["Ari","Aries"],["Aur","Auriga"],["Boo","Bootes"],["Cae","Caelum"],["Cam","Camelopardis"],["Cap","Capricornus"],["Car","Carina"],["Cas","Cassiopeia"],["Cen","Centaurus"],["Cep","Cepheus"],["Cet","Cetus"],["Cha","Chamaeleon"],["Cir",
+"Circinus"],["CMa","Canis Major"],["CMi","Canis Minor"],["Cnc","Cancer"],["Col","Columba"],["Com","Coma Berenices"],["CrA","Corona Australis"],["CrB","Corona Borealis"],["Crt","Crater"],["Cru","Crux"],["Crv","Corvus"],["CVn","Canes Venatici"],["Cyg","Cygnus"],["Del","Delphinus"],["Dor","Dorado"],["Dra","Draco"],["Equ","Equuleus"],["Eri","Eridanus"],["For","Fornax"],["Gem","Gemini"],["Gru","Grus"],["Her","Hercules"],["Hor","Horologium"],["Hya","Hydra"],["Hyi","Hydrus"],["Ind","Indus"],["Lac","Lacerta"],
+["Leo","Leo"],["Lep","Lepus"],["Lib","Libra"],["LMi","Leo Minor"],["Lup","Lupus"],["Lyn","Lynx"],["Lyr","Lyra"],["Men","Mensa"],["Mic","Microscopium"],["Mon","Monoceros"],["Mus","Musca"],["Nor","Norma"],["Oct","Octans"],["Oph","Ophiuchus"],["Ori","Orion"],["Pav","Pavo"],["Peg","Pegasus"],["Per","Perseus"],["Phe","Phoenix"],["Pic","Pictor"],["PsA","Pisces Austrinus"],["Psc","Pisces"],["Pup","Puppis"],["Pyx","Pyxis"],["Ret","Reticulum"],["Scl","Sculptor"],["Sco","Scorpius"],["Sct","Scutum"],["Ser",
+"Serpens"],["Sex","Sextans"],["Sge","Sagitta"],["Sgr","Sagittarius"],["Tau","Taurus"],["Tel","Telescopium"],["TrA","Triangulum Australe"],["Tri","Triangulum"],["Tuc","Tucana"],["UMa","Ursa Major"],["UMi","Ursa Minor"],["Vel","Vela"],["Vir","Virgo"],["Vol","Volans"],["Vul","Vulpecula"]],Hc=[[83,0,8640,2112],[83,2880,5220,2076],[83,7560,8280,2068],[83,6480,7560,2064],[15,0,2880,2040],[10,3300,3840,1968],[15,0,1800,1920],[10,3840,5220,1920],[83,6300,6480,1920],[33,7260,7560,1920],[15,0,1263,1848],[10,
+4140,4890,1848],[83,5952,6300,1800],[15,7260,7440,1800],[10,2868,3300,1764],[33,3300,4080,1764],[83,4680,5952,1680],[13,1116,1230,1632],[33,7350,7440,1608],[33,4080,4320,1596],[15,0,120,1584],[83,5040,5640,1584],[15,8490,8640,1584],[33,4320,4860,1536],[33,4860,5190,1512],[15,8340,8490,1512],[10,2196,2520,1488],[33,7200,7350,1476],[15,7393.2,7416,1462],[10,2520,2868,1440],[82,2868,3030,1440],[33,7116,7200,1428],[15,7200,7393.2,1428],[15,8232,8340,1418],[13,0,876,1404],[33,6990,7116,1392],[13,612,687,
+1380],[13,876,1116,1368],[10,1116,1140,1368],[15,8034,8232,1350],[10,1800,2196,1344],[82,5052,5190,1332],[33,5190,6990,1332],[10,1140,1200,1320],[15,7968,8034,1320],[15,7416,7908,1316],[13,0,612,1296],[50,2196,2340,1296],[82,4350,4860,1272],[33,5490,5670,1272],[15,7908,7968,1266],[10,1200,1800,1260],[13,8232,8400,1260],[33,5670,6120,1236],[62,735,906,1212],[33,6120,6564,1212],[13,0,492,1200],[62,492,600,1200],[50,2340,2448,1200],[13,8400,8640,1200],[82,4860,5052,1164],[13,0,402,1152],[13,8490,8640,
+1152],[39,6543,6564,1140],[33,6564,6870,1140],[30,6870,6900,1140],[62,600,735,1128],[82,3030,3300,1128],[13,60,312,1104],[82,4320,4350,1080],[50,2448,2652,1068],[30,7887,7908,1056],[30,7875,7887,1050],[30,6900,6984,1044],[82,3300,3660,1008],[82,3660,3882,960],[8,5556,5670,960],[39,5670,5880,960],[50,3330,3450,954],[0,0,906,882],[62,906,924,882],[51,6969,6984,876],[62,1620,1689,864],[30,7824,7875,864],[44,7875,7920,864],[7,2352,2652,852],[50,2652,2790,852],[0,0,720,840],[44,7920,8214,840],[44,8214,
+8232,828],[0,8232,8460,828],[62,924,978,816],[82,3882,3960,816],[29,4320,4440,816],[50,2790,3330,804],[48,3330,3558,804],[0,258,507,792],[8,5466,5556,792],[0,8460,8550,770],[29,4440,4770,768],[0,8550,8640,752],[29,5025,5052,738],[80,870,978,736],[62,978,1620,736],[7,1620,1710,720],[51,6543,6969,720],[82,3960,4320,696],[30,7080,7530,696],[7,1710,2118,684],[48,3558,3780,684],[29,4770,5025,684],[0,0,24,672],[80,507,600,672],[7,2118,2352,672],[37,2838,2880,672],[30,7530,7824,672],[30,6933,7080,660],[80,
+690,870,654],[25,5820,5880,648],[8,5430,5466,624],[25,5466,5820,624],[51,6612,6792,624],[48,3870,3960,612],[51,6792,6933,612],[80,600,690,600],[66,258,306,570],[48,3780,3870,564],[87,7650,7710,564],[77,2052,2118,548],[0,24,51,528],[73,5730,5772,528],[37,2118,2238,516],[87,7140,7290,510],[87,6792,6930,506],[0,51,306,504],[87,7290,7404,492],[37,2811,2838,480],[87,7404,7650,468],[87,6930,7140,460],[6,1182,1212,456],[75,6792,6840,444],[59,2052,2076,432],[37,2238,2271,420],[75,6840,7140,388],[77,1788,
+1920,384],[39,5730,5790,384],[75,7140,7290,378],[77,1662,1788,372],[77,1920,2016,372],[23,4620,4860,360],[39,6210,6570,344],[23,4272,4620,336],[37,2700,2811,324],[39,6030,6210,308],[61,0,51,300],[77,2016,2076,300],[37,2520,2700,300],[61,7602,7680,300],[37,2271,2496,288],[39,6570,6792,288],[31,7515,7578,284],[61,7578,7602,284],[45,4146,4272,264],[59,2247,2271,240],[37,2496,2520,240],[21,2811,2853,240],[61,8580,8640,240],[6,600,1182,238],[31,7251,7308,204],[8,4860,5430,192],[61,8190,8580,180],[21,2853,
+3330,168],[45,3330,3870,168],[58,6570,6718.4,150],[3,6718.4,6792,150],[31,7500,7515,144],[20,2520,2526,132],[73,6570,6633,108],[39,5790,6030,96],[58,6570,6633,72],[61,7728,7800,66],[66,0,720,48],[73,6690,6792,48],[31,7308,7500,48],[34,7500,7680,48],[61,7680,7728,48],[61,7920,8190,48],[61,7800,7920,42],[20,2526,2592,36],[77,1290,1662,0],[59,1662,1680,0],[20,2592,2910,0],[85,5280,5430,0],[58,6420,6570,0],[16,954,1182,-42],[77,1182,1290,-42],[73,5430,5856,-78],[59,1680,1830,-96],[59,2100,2247,-96],[73,
+6420,6468,-96],[73,6570,6690,-96],[3,6690,6792,-96],[66,8190,8580,-96],[45,3870,4146,-144],[85,4146,4260,-144],[66,0,120,-168],[66,8580,8640,-168],[85,5130,5280,-192],[58,5730,5856,-192],[3,7200,7392,-216],[4,7680,7872,-216],[58,6180,6468,-240],[54,2100,2910,-264],[35,1770,1830,-264],[59,1830,2100,-264],[41,2910,3012,-264],[74,3450,3870,-264],[85,4260,4620,-264],[58,6330,6360,-280],[3,6792,7200,-288.8],[35,1740,1770,-348],[4,7392,7680,-360],[73,6180,6570,-384],[72,6570,6792,-384],[41,3012,3090,-408],
+[58,5856,5895,-438],[41,3090,3270,-456],[26,3870,3900,-456],[71,5856,5895,-462],[47,5640,5730,-480],[28,4530,4620,-528],[85,4620,5130,-528],[41,3270,3510,-576],[16,600,954,-585.2],[35,954,1350,-585.2],[26,3900,4260,-588],[28,4260,4530,-588],[47,5130,5370,-588],[58,5856,6030,-590],[16,0,600,-612],[11,7680,7872,-612],[4,7872,8580,-612],[16,8580,8640,-612],[41,3510,3690,-636],[35,1692,1740,-654],[46,1740,2202,-654],[11,7200,7680,-672],[41,3690,3810,-700],[41,4530,5370,-708],[47,5370,5640,-708],[71,5640,
+5760,-708],[35,1650,1692,-720],[58,6030,6336,-720],[76,6336,6420,-720],[41,3810,3900,-748],[19,2202,2652,-792],[41,4410,4530,-792],[41,3900,4410,-840],[36,1260,1350,-864],[68,3012,3372,-882],[35,1536,1650,-888],[76,6420,6900,-888],[65,7680,8280,-888],[70,8280,8400,-888],[36,1080,1260,-950],[1,3372,3960,-954],[70,0,600,-960],[36,600,1080,-960],[35,1392,1536,-960],[70,8400,8640,-960],[14,5100,5370,-1008],[49,5640,5760,-1008],[71,5760,5911.5,-1008],[9,1740,1800,-1032],[22,1800,2370,-1032],[67,2880,3012,
+-1032],[35,1230,1392,-1056],[71,5911.5,6420,-1092],[24,6420,6900,-1092],[76,6900,7320,-1092],[53,7320,7680,-1092],[35,1080,1230,-1104],[9,1620,1740,-1116],[49,5520,5640,-1152],[63,0,840,-1156],[35,960,1080,-1176],[40,1470,1536,-1176],[9,1536,1620,-1176],[38,7680,7920,-1200],[67,2160,2880,-1218],[84,2880,2940,-1218],[35,870,960,-1224],[40,1380,1470,-1224],[63,0,660,-1236],[12,2160,2220,-1260],[84,2940,3042,-1272],[40,1260,1380,-1276],[32,1380,1440,-1276],[63,0,570,-1284],[35,780,870,-1296],[64,1620,
+1800,-1296],[49,5418,5520,-1296],[84,3042,3180,-1308],[12,2220,2340,-1320],[14,4260,4620,-1320],[49,5100,5418,-1320],[56,5418,5520,-1320],[32,1440,1560,-1356],[84,3180,3960,-1356],[14,3960,4050,-1356],[5,6300,6480,-1368],[78,6480,7320,-1368],[38,7920,8400,-1368],[40,1152,1260,-1380],[64,1800,1980,-1380],[12,2340,2460,-1392],[63,0,480,-1404],[35,480,780,-1404],[63,8400,8640,-1404],[32,1560,1650,-1416],[56,5520,5911.5,-1440],[43,7320,7680,-1440],[64,1980,2160,-1464],[18,5460,5520,-1464],[5,5911.5,5970,
+-1464],[18,5370,5460,-1526],[5,5970,6030,-1526],[64,2160,2460,-1536],[12,2460,3252,-1536],[14,4050,4260,-1536],[27,4260,4620,-1536],[14,4620,5232,-1536],[18,4860,4920,-1560],[5,6030,6060,-1560],[40,780,1152,-1620],[69,1152,1650,-1620],[18,5310,5370,-1620],[5,6060,6300,-1620],[60,6300,6480,-1620],[81,7920,8400,-1620],[32,1650,2370,-1680],[18,4920,5310,-1680],[79,5310,6120,-1680],[81,0,480,-1800],[42,1260,1650,-1800],[86,2370,3252,-1800],[12,3252,4050,-1800],[55,4050,4920,-1800],[60,6480,7680,-1800],
+[43,7680,8400,-1800],[81,8400,8640,-1800],[81,270,480,-1824],[42,0,1260,-1980],[17,2760,4920,-1980],[2,4920,6480,-1980],[52,1260,2760,-2040],[57,0,8640,-2160]],qb,sc,tc=function(a,b,c,d){this.symbol=a;this.name=b;this.ra1875=c;this.dec1875=d};h.ConstellationInfo=tc;h.Constellation=function(a,b){r(a);r(b);if(-90>b||90a&&(a+=24);qb||(qb=kb(new P(-45655.74141261017)),sc=new P(0));a=new Ra(b,15*a,1);a=ib(a,sc);a=Aa(qb,a);a=Vb(a);b=10/240;
+for(var c=b/15,d=$jscomp.makeIterator(Hc),e=d.next();!e.done;e=d.next()){e=e.value;var f=e[1]*c,k=e[2]*c;if(e[3]*b<=a.dec&&f<=a.ra&&a.raMath.abs(c))throw"AngleBetween: first vector is too short.";var d=b.x*b.x+b.y*b.y+b.z*b.z;if(1E-8>Math.abs(d))throw"AngleBetween: second vector is too short.";a=(a.x*b.x+a.y*b.y+a.z*b.z)/Math.sqrt(c*d);return-1>=a?180:1<=a?0:RAD2DEG*Math.acos(a)}exports.AngleBetween=AngleBetween;exports.Bodies="Sun Moon Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune Pluto SSB EMB".split(" ");
var Planet={Mercury:{OrbitalPeriod:87.969},Venus:{OrbitalPeriod:224.701},Earth:{OrbitalPeriod:365.256},Mars:{OrbitalPeriod:686.98},Jupiter:{OrbitalPeriod:4332.589},Saturn:{OrbitalPeriod:10759.22},Uranus:{OrbitalPeriod:30685.4},Neptune:{OrbitalPeriod:60189},Pluto:{OrbitalPeriod:90560}},vsop={Mercury:[[[[4.40250710144,0,0],[.40989414977,1.48302034195,26087.9031415742],[.050462942,4.47785489551,52175.8062831484],[.00855346844,1.16520322459,78263.70942472259],[.00165590362,4.11969163423,104351.61256629678],
[3.4561897E-4,.77930768443,130439.51570787099],[7.583476E-5,3.71348404924,156527.41884944518]],[[26087.90313685529,0,0],[.01131199811,6.21874197797,26087.9031415742],[.00292242298,3.04449355541,52175.8062831484],[7.5775081E-4,6.08568821653,78263.70942472259],[1.9676525E-4,2.80965111777,104351.61256629678]]],[[[.11737528961,1.98357498767,26087.9031415742],[.02388076996,5.03738959686,52175.8062831484],[.01222839532,3.14159265359,0],[.0054325181,1.79644363964,78263.70942472259],[.0012977877,4.83232503958,
@@ -199,7 +198,7 @@ function InverseRotation(a){return new RotationMatrix([[a.rot[0][0],a.rot[1][0],
function CombineRotation(a,b){return new RotationMatrix([[b.rot[0][0]*a.rot[0][0]+b.rot[1][0]*a.rot[0][1]+b.rot[2][0]*a.rot[0][2],b.rot[0][1]*a.rot[0][0]+b.rot[1][1]*a.rot[0][1]+b.rot[2][1]*a.rot[0][2],b.rot[0][2]*a.rot[0][0]+b.rot[1][2]*a.rot[0][1]+b.rot[2][2]*a.rot[0][2]],[b.rot[0][0]*a.rot[1][0]+b.rot[1][0]*a.rot[1][1]+b.rot[2][0]*a.rot[1][2],b.rot[0][1]*a.rot[1][0]+b.rot[1][1]*a.rot[1][1]+b.rot[2][1]*a.rot[1][2],b.rot[0][2]*a.rot[1][0]+b.rot[1][2]*a.rot[1][1]+b.rot[2][2]*a.rot[1][2]],[b.rot[0][0]*
a.rot[2][0]+b.rot[1][0]*a.rot[2][1]+b.rot[2][0]*a.rot[2][2],b.rot[0][1]*a.rot[2][0]+b.rot[1][1]*a.rot[2][1]+b.rot[2][1]*a.rot[2][2],b.rot[0][2]*a.rot[2][0]+b.rot[1][2]*a.rot[2][1]+b.rot[2][2]*a.rot[2][2]]])}exports.CombineRotation=CombineRotation;function IdentityMatrix(){return new RotationMatrix([[1,0,0],[0,1,0],[0,0,1]])}exports.IdentityMatrix=IdentityMatrix;
function Pivot(a,b,c){if(0!==b&&1!==b&&2!==b)throw"Invalid axis "+b+". Must be [0, 1, 2].";var d=VerifyNumber(c)*DEG2RAD;c=Math.cos(d);d=Math.sin(d);var e=(b+1)%3,f=(b+2)%3,g=[[0,0,0],[0,0,0],[0,0,0]];g[e][e]=c*a.rot[e][e]-d*a.rot[e][f];g[e][f]=d*a.rot[e][e]+c*a.rot[e][f];g[e][b]=a.rot[e][b];g[f][e]=c*a.rot[f][e]-d*a.rot[f][f];g[f][f]=d*a.rot[f][e]+c*a.rot[f][f];g[f][b]=a.rot[f][b];g[b][e]=c*a.rot[b][e]-d*a.rot[b][f];g[b][f]=d*a.rot[b][e]+c*a.rot[b][f];g[b][b]=a.rot[b][b];return new RotationMatrix(g)}
-exports.Pivot=Pivot;function VectorFromSphere(a,b){var c=a.lat*DEG2RAD,d=a.lon*DEG2RAD,e=a.dist*Math.cos(c);return new Vector(e*Math.cos(d),e*Math.sin(d),a.dist*Math.sin(c),b)}exports.VectorFromSphere=VectorFromSphere;function VectorFromEquator(a,b){return VectorFromSphere(new Spherical(a.dec,15*a.ra,a.dist),b)}exports.VectorFromEquator=VectorFromEquator;function EquatorFromVector(a){var b=SphereFromVector(a);return new EquatorialCoordinates(b.lon/15,b.lat,b.dist,a)}exports.EquatorFromVector=EquatorFromVector;
+exports.Pivot=Pivot;function VectorFromSphere(a,b){var c=a.lat*DEG2RAD,d=a.lon*DEG2RAD,e=a.dist*Math.cos(c);return new Vector(e*Math.cos(d),e*Math.sin(d),a.dist*Math.sin(c),b)}exports.VectorFromSphere=VectorFromSphere;function EquatorFromVector(a){var b=SphereFromVector(a);return new EquatorialCoordinates(b.lon/15,b.lat,b.dist,a)}exports.EquatorFromVector=EquatorFromVector;
function SphereFromVector(a){var b=a.x*a.x+a.y*a.y,c=Math.sqrt(b+a.z*a.z);if(0===b){if(0===a.z)throw"Zero-length vector not allowed.";var d=0;a=0>a.z?-90:90}else d=RAD2DEG*Math.atan2(a.y,a.x),0>d&&(d+=360),a=RAD2DEG*Math.atan2(a.z,Math.sqrt(b));return new Spherical(a,d,c)}exports.SphereFromVector=SphereFromVector;function ToggleAzimuthDirection(a){a=360-a;360<=a?a-=360:0>a&&(a+=360);return a}
function HorizonFromVector(a,b){a=SphereFromVector(a);a.lon=ToggleAzimuthDirection(a.lon);a.lat+=Refraction(b,a.lat);return a}exports.HorizonFromVector=HorizonFromVector;function VectorFromHorizon(a,b,c){var d=ToggleAzimuthDirection(a.lon);c=a.lat+InverseRefraction(c,a.lat);a=new Spherical(c,d,a.dist);return VectorFromSphere(a,b)}exports.VectorFromHorizon=VectorFromHorizon;
function Refraction(a,b){VerifyNumber(b);if(-90>b||90c&&(c=-1);c=1.02/Math.tan((c+10.3/(c+5.11))*DEG2RAD)/60;"normal"===a&&-1>b&&(c*=(b+90)/89)}else c=0;return c}exports.Refraction=Refraction;function InverseRefraction(a,b){if(-90>b||90Math.abs(d))return c-b;c-=d}}exports.InverseRefraction=InverseRefraction;
@@ -226,8 +225,8 @@ var ConstelNames=[["And","Andromeda"],["Ant","Antila"],["Aps","Apus"],["Aql","Aq
[32,1440,1560,-1356],[84,3180,3960,-1356],[14,3960,4050,-1356],[5,6300,6480,-1368],[78,6480,7320,-1368],[38,7920,8400,-1368],[40,1152,1260,-1380],[64,1800,1980,-1380],[12,2340,2460,-1392],[63,0,480,-1404],[35,480,780,-1404],[63,8400,8640,-1404],[32,1560,1650,-1416],[56,5520,5911.5,-1440],[43,7320,7680,-1440],[64,1980,2160,-1464],[18,5460,5520,-1464],[5,5911.5,5970,-1464],[18,5370,5460,-1526],[5,5970,6030,-1526],[64,2160,2460,-1536],[12,2460,3252,-1536],[14,4050,4260,-1536],[27,4260,4620,-1536],[14,
4620,5232,-1536],[18,4860,4920,-1560],[5,6030,6060,-1560],[40,780,1152,-1620],[69,1152,1650,-1620],[18,5310,5370,-1620],[5,6060,6300,-1620],[60,6300,6480,-1620],[81,7920,8400,-1620],[32,1650,2370,-1680],[18,4920,5310,-1680],[79,5310,6120,-1680],[81,0,480,-1800],[42,1260,1650,-1800],[86,2370,3252,-1800],[12,3252,4050,-1800],[55,4050,4920,-1800],[60,6480,7680,-1800],[43,7680,8400,-1800],[81,8400,8640,-1800],[81,270,480,-1824],[42,0,1260,-1980],[17,2760,4920,-1980],[2,4920,6480,-1980],[52,1260,2760,
-2040],[57,0,8640,-2160]],ConstelRot,Epoch2000,ConstellationInfo=function(a,b,c,d){this.symbol=a;this.name=b;this.ra1875=c;this.dec1875=d};exports.ConstellationInfo=ConstellationInfo;
-function Constellation(a,b){VerifyNumber(a);VerifyNumber(b);if(-90>b||90a&&(a+=24);ConstelRot||(ConstelRot=Rotation_EQJ_EQD(new AstroTime(-45655.74141261017)),Epoch2000=new AstroTime(0));var c=new Vector(0,0,0,Epoch2000);a=new EquatorialCoordinates(a,b,1,c);a=VectorFromEquator(a,Epoch2000);a=RotateVector(ConstelRot,a);a=EquatorFromVector(a);b=10/240;c=b/15;for(var d=$jscomp.makeIterator(ConstelBounds),e=d.next();!e.done;e=d.next()){e=
-e.value;var f=e[1]*c,g=e[2]*c;if(e[3]*b<=a.dec&&f<=a.ra&&a.rab||90a&&(a+=24);ConstelRot||(ConstelRot=Rotation_EQJ_EQD(new AstroTime(-45655.74141261017)),Epoch2000=new AstroTime(0));a=new Spherical(b,15*a,1);a=VectorFromSphere(a,Epoch2000);a=RotateVector(ConstelRot,a);a=EquatorFromVector(a);b=10/240;for(var c=b/15,d=$jscomp.makeIterator(ConstelBounds),e=d.next();!e.done;e=d.next()){e=e.value;var f=e[1]*c,g=e[2]*c;if(e[3]*b<=a.dec&&
+f<=a.ra&&a.ra
-### VectorFromEquator(equ, time)
-
-**Given angular equatorial coordinates in `equ`, calculates equatorial vector.**
-
-| Type | Parameter | Description |
-| --- | --- | --- |
-| [`Equatorial`](#Equatorial) | `equ` | Angular equatorial coordinates to be converted to a vector. |
-| [`Time`](#Time) | `time` | The date and time of the observation. This is needed because the returned vector object requires a valid time value when passed to certain other functions. |
-
-### Returns: [`Vector`](#Vector)
-A vector in the equatorial system.
-
----
-
### VectorFromHorizon(sphere, time, refraction)
diff --git a/source/python/astronomy.py b/source/python/astronomy.py
index 56978617..8a0c7d1d 100644
--- a/source/python/astronomy.py
+++ b/source/python/astronomy.py
@@ -5720,25 +5720,6 @@ def VectorFromSphere(sphere, time):
)
-def VectorFromEquator(equ, time):
- """Given angular equatorial coordinates in `equ`, calculates equatorial vector.
-
- Parameters
- ----------
- equ : Equatorial
- Angular equatorial coordinates to be converted to a vector.
- time : Time
- The date and time of the observation. This is needed because the returned
- vector object requires a valid time value when passed to certain other functions.
-
- Returns
- -------
- Vector
- A vector in the equatorial system.
- """
- return VectorFromSphere(Spherical(equ.dec, 15.0 * equ.ra, equ.dist), time)
-
-
def EquatorFromVector(vec):
"""Given an equatorial vector, calculates equatorial angular coordinates.
@@ -6883,8 +6864,8 @@ def Constellation(ra, dec):
_Epoch2000 = Time(0.0)
# Convert coordinates from J2000 to B1875.
- equ2000 = Equatorial(ra, dec, 1.0, None) # FIXFIXFIX - avoid this hack with unused vector
- vec2000 = VectorFromEquator(equ2000, _Epoch2000)
+ sph2000 = Spherical(dec, 15.0 * ra, 1.0)
+ vec2000 = VectorFromSphere(sph2000, _Epoch2000)
vec1875 = RotateVector(_ConstelRot, vec2000)
equ1875 = EquatorFromVector(vec1875)
diff --git a/website/src/assets/documentation.json b/website/src/assets/documentation.json
index 58de360f..22967d00 100644
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- "paramnames": []
- }
- },
- "undocumented": true,
- "name": "VectorFromEquator",
- "longname": "NextTransit#TransitInfo#SearchLocalSolarEclipse#EclipseEvent#SearchGlobalSolarEclipse#GlobalSolarEclipseInfo#LunarEclipseInfo#ConstellationInfo#Rotation_ECL_HOR#Rotation_EQD_ECL#Rotation_HOR_EQJ#Rotation_EQD_HOR#Rotation_EQJ_EQD#Rotation_EQJ_ECL#InverseRefraction#VectorFromHorizon#SphereFromVector#VectorFromEquator",
- "kind": "member",
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"lineno": 1754,
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@@ -18860,14 +18835,14 @@
"comment": "/**\n * @brief Represents the location of an object seen by an observer on the Earth.\n *\n * Holds azimuth (compass direction) and altitude (angle above/below the horizon)\n * of a celestial object as seen by an observer at a particular location on the Earth's surface.\n * Also holds right ascension and declination of the same object.\n * All of these coordinates are optionally adjusted for atmospheric refraction;\n * therefore the right ascension and declination values may not exactly match\n * those found inside a corresponding {@link EquatorialCoordinates} object.\n *\n * @property {number} azimuth\n * A horizontal compass direction angle in degrees measured starting at north\n * and increasing positively toward the east.\n * The value is in the range [0, 360).\n * North = 0, east = 90, south = 180, west = 270.\n *\n * @property {number} altitude\n * A vertical angle in degrees above (positive) or below (negative) the horizon.\n * The value is in the range [-90, +90].\n * The altitude angle is optionally adjusted upward due to atmospheric refraction.\n *\n * @property {number} ra\n * The right ascension of the celestial body in sidereal hours.\n * The value is in the reange [0, 24).\n * If `altitude` was adjusted for atmospheric reaction, `ra`\n * is likewise adjusted.\n *\n * @property {number} dec\n * The declination of of the celestial body in degrees.\n * The value in the range [-90, +90].\n * If `altitude` was adjusted for atmospheric reaction, `dec`\n * is likewise adjusted.\n */",
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"lineno": 1788,
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"lineno": 1789,
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+ "id": "astnode100009862",
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@@ -18966,14 +18941,14 @@
"comment": "/**\n * @brief Represents the location of an object seen by an observer on the Earth.\n *\n * Holds azimuth (compass direction) and altitude (angle above/below the horizon)\n * of a celestial object as seen by an observer at a particular location on the Earth's surface.\n * Also holds right ascension and declination of the same object.\n * All of these coordinates are optionally adjusted for atmospheric refraction;\n * therefore the right ascension and declination values may not exactly match\n * those found inside a corresponding {@link EquatorialCoordinates} object.\n *\n * @property {number} azimuth\n * A horizontal compass direction angle in degrees measured starting at north\n * and increasing positively toward the east.\n * The value is in the range [0, 360).\n * North = 0, east = 90, south = 180, west = 270.\n *\n * @property {number} altitude\n * A vertical angle in degrees above (positive) or below (negative) the horizon.\n * The value is in the range [-90, +90].\n * The altitude angle is optionally adjusted upward due to atmospheric refraction.\n *\n * @property {number} ra\n * The right ascension of the celestial body in sidereal hours.\n * The value is in the reange [0, 24).\n * If `altitude` was adjusted for atmospheric reaction, `ra`\n * is likewise adjusted.\n *\n * @property {number} dec\n * The declination of of the celestial body in degrees.\n * The value in the range [-90, +90].\n * If `altitude` was adjusted for atmospheric reaction, `dec`\n * is likewise adjusted.\n */",
"meta": {
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"lineno": 1788,
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"comment": "",
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"filename": "astronomy.js",
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@@ -19089,14 +19064,14 @@
"comment": "",
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"filename": "astronomy.js",
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"comment": "",
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"filename": "astronomy.js",
"lineno": 1793,
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@@ -19139,14 +19114,14 @@
"comment": "",
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"filename": "astronomy.js",
"lineno": 1796,
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"code": {
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+ "id": "astnode100009903",
"name": "exports.HorizontalCoordinates",
"type": "Identifier",
"value": "HorizontalCoordinates",
@@ -19163,14 +19138,14 @@
"comment": "/**\n * @brief Ecliptic coordinates of a celestial body.\n *\n * The origin and date of the coordinate system may vary depending on the caller's usage.\n * In general, ecliptic coordinates are measured with respect to the mean plane of the Earth's\n * orbit around the Sun.\n * Includes Cartesian coordinates `(ex, ey, ez)` measured in\n * astronomical units (AU)\n * and spherical coordinates `(elon, elat)` measured in degrees.\n *\n * @property {number} ex\n * The Cartesian x-coordinate of the body in astronomical units (AU).\n * The x-axis is within the ecliptic plane and is oriented in the direction of the\n * equinox.\n *\n * @property {number} ey\n * The Cartesian y-coordinate of the body in astronomical units (AU).\n * The y-axis is within the ecliptic plane and is oriented 90 degrees\n * counterclockwise from the equinox, as seen from above the Sun's north pole.\n *\n * @property {number} ez\n * The Cartesian z-coordinate of the body in astronomical units (AU).\n * The z-axis is oriented perpendicular to the ecliptic plane,\n * along the direction of the Sun's north pole.\n *\n * @property {number} elat\n * The ecliptic latitude of the body in degrees.\n * This is the angle north or south of the ecliptic plane.\n * The value is in the range [-90, +90].\n * Positive values are north and negative values are south.\n *\n * @property {number} elon\n * The ecliptic longitude of the body in degrees.\n * This is the angle measured counterclockwise around the ecliptic plane,\n * as seen from above the Sun's north pole.\n * This is the same direction that the Earth orbits around the Sun.\n * The angle is measured starting at 0 from the equinox and increases\n * up to 360 degrees.\n */",
"meta": {
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"filename": "astronomy.js",
"lineno": 1836,
"columnno": 0,
"code": {
- "id": "astnode100009912",
+ "id": "astnode100009908",
"name": "EclipticCoordinates",
"type": "ClassDeclaration",
"paramnames": [
@@ -19247,14 +19222,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
"lineno": 1837,
"columnno": 4,
"code": {
- "id": "astnode100009915",
+ "id": "astnode100009911",
"name": "EclipticCoordinates",
"type": "MethodDefinition",
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@@ -19280,14 +19255,14 @@
"comment": "/**\n * @brief Ecliptic coordinates of a celestial body.\n *\n * The origin and date of the coordinate system may vary depending on the caller's usage.\n * In general, ecliptic coordinates are measured with respect to the mean plane of the Earth's\n * orbit around the Sun.\n * Includes Cartesian coordinates `(ex, ey, ez)` measured in\n * astronomical units (AU)\n * and spherical coordinates `(elon, elat)` measured in degrees.\n *\n * @property {number} ex\n * The Cartesian x-coordinate of the body in astronomical units (AU).\n * The x-axis is within the ecliptic plane and is oriented in the direction of the\n * equinox.\n *\n * @property {number} ey\n * The Cartesian y-coordinate of the body in astronomical units (AU).\n * The y-axis is within the ecliptic plane and is oriented 90 degrees\n * counterclockwise from the equinox, as seen from above the Sun's north pole.\n *\n * @property {number} ez\n * The Cartesian z-coordinate of the body in astronomical units (AU).\n * The z-axis is oriented perpendicular to the ecliptic plane,\n * along the direction of the Sun's north pole.\n *\n * @property {number} elat\n * The ecliptic latitude of the body in degrees.\n * This is the angle north or south of the ecliptic plane.\n * The value is in the range [-90, +90].\n * Positive values are north and negative values are south.\n *\n * @property {number} elon\n * The ecliptic longitude of the body in degrees.\n * This is the angle measured counterclockwise around the ecliptic plane,\n * as seen from above the Sun's north pole.\n * This is the same direction that the Earth orbits around the Sun.\n * The angle is measured starting at 0 from the equinox and increases\n * up to 360 degrees.\n */",
"meta": {
"range": [
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],
"filename": "astronomy.js",
"lineno": 1836,
"columnno": 0,
"code": {
- "id": "astnode100009912",
+ "id": "astnode100009908",
"name": "EclipticCoordinates",
"type": "ClassDeclaration",
"paramnames": [
@@ -19363,14 +19338,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
"lineno": 1838,
"columnno": 8,
"code": {
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"type": "CallExpression",
"value": "",
@@ -19388,14 +19363,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
"lineno": 1839,
"columnno": 8,
"code": {
- "id": "astnode100009933",
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"name": "this.ey",
"type": "CallExpression",
"value": "",
@@ -19413,14 +19388,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
"lineno": 1840,
"columnno": 8,
"code": {
- "id": "astnode100009941",
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"name": "this.ez",
"type": "CallExpression",
"value": "",
@@ -19438,14 +19413,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
"lineno": 1841,
"columnno": 8,
"code": {
- "id": "astnode100009949",
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"name": "this.elat",
"type": "CallExpression",
"value": "",
@@ -19463,14 +19438,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
"lineno": 1842,
"columnno": 8,
"code": {
- "id": "astnode100009957",
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"name": "this.elon",
"type": "CallExpression",
"value": "",
@@ -19488,14 +19463,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
"lineno": 1845,
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"code": {
- "id": "astnode100009965",
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"name": "exports.EclipticCoordinates",
"type": "Identifier",
"value": "EclipticCoordinates",
@@ -19512,14 +19487,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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- "id": "astnode100009970",
+ "id": "astnode100009966",
"name": "vector2radec",
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@@ -19546,14 +19521,14 @@
"comment": "",
"meta": {
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],
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@@ -19571,14 +19546,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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@@ -19596,14 +19571,14 @@
"comment": "",
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],
"filename": "astronomy.js",
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@@ -19621,14 +19596,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"value": ""
@@ -19646,14 +19621,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
"lineno": 1859,
"columnno": 8,
"code": {
- "id": "astnode100010081",
+ "id": "astnode100010077",
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"type": "Literal",
"funcscope": "vector2radec",
@@ -19672,14 +19647,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
"lineno": 1860,
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@@ -19697,14 +19672,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
"lineno": 1863,
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"code": {
- "id": "astnode100010108",
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"name": "spin",
"type": "FunctionDeclaration",
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@@ -19738,14 +19713,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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@@ -19763,14 +19738,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
"lineno": 1865,
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@@ -19788,14 +19763,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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@@ -19813,14 +19788,14 @@
"comment": "",
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],
"filename": "astronomy.js",
"lineno": 1867,
"columnno": 10,
"code": {
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"name": "xx",
"type": "Identifier",
"value": "cosang"
@@ -19838,14 +19813,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
"lineno": 1868,
"columnno": 10,
"code": {
- "id": "astnode100010140",
+ "id": "astnode100010136",
"name": "yx",
"type": "Identifier",
"value": "sinang"
@@ -19863,14 +19838,14 @@
"comment": "",
"meta": {
"range": [
- 84444,
- 84450
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],
"filename": "astronomy.js",
"lineno": 1869,
"columnno": 10,
"code": {
- "id": "astnode100010144",
+ "id": "astnode100010140",
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@@ -19888,14 +19863,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
"lineno": 1870,
"columnno": 10,
"code": {
- "id": "astnode100010148",
+ "id": "astnode100010144",
"name": "xy",
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"value": "-sinang"
@@ -19913,14 +19888,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
"lineno": 1871,
"columnno": 10,
"code": {
- "id": "astnode100010153",
+ "id": "astnode100010149",
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"type": "Identifier",
"value": "cosang"
@@ -19938,14 +19913,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
"lineno": 1872,
"columnno": 10,
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- "id": "astnode100010157",
+ "id": "astnode100010153",
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@@ -19963,14 +19938,14 @@
"comment": "",
"meta": {
"range": [
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- 84533
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+ 84505
],
"filename": "astronomy.js",
"lineno": 1873,
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- "id": "astnode100010161",
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@@ -19988,14 +19963,14 @@
"comment": "",
"meta": {
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],
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@@ -20013,14 +19988,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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@@ -20038,14 +20013,14 @@
"comment": "/**\n * @brief Converts equatorial coordinates to horizontal coordinates.\n *\n * Given a date and time, a geographic location of an observer on the Earth, and\n * equatorial coordinates (right ascension and declination) of a celestial body,\n * returns horizontal coordinates (azimuth and altitude angles) for that body\n * as seen by that observer. Allows optional correction for atmospheric refraction.\n *\n * @param {FlexibleDateTime} date\n * The date and time for which to find horizontal coordinates.\n *\n * @param {Observer} observer\n * The location of the observer for which to find horizontal coordinates.\n *\n * @param {number} ra\n * Right ascension in sidereal hours of the celestial object,\n * referred to the mean equinox of date for the J2000 epoch.\n *\n * @param {number} dec\n * Declination in degrees of the celestial object,\n * referred to the mean equator of date for the J2000 epoch.\n * Positive values are north of the celestial equator and negative values are south.\n *\n * @param {string} refraction\n * If omitted or has a false-like value (false, null, undefined, etc.)\n * the calculations are performed without any correction for atmospheric\n * refraction. If the value is the string `\"normal\"`,\n * uses the recommended refraction correction based on Meeus \"Astronomical Algorithms\"\n * with a linear taper more than 1 degree below the horizon. The linear\n * taper causes the refraction to linearly approach 0 as the altitude of the\n * body approaches the nadir (-90 degrees).\n * If the value is the string `\"jplhor\"`, uses a JPL Horizons\n * compatible formula. This is the same algorithm as `\"normal\"`,\n * only without linear tapering; this can result in physically impossible\n * altitudes of less than -90 degrees, which may cause problems for some applications.\n * (The `\"jplhor\"` option was created for unit testing against data\n * generated by JPL Horizons, and is otherwise not recommended for use.)\n *\n * @returns {HorizontalCoordinates}\n */",
"meta": {
"range": [
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],
"filename": "astronomy.js",
"lineno": 1922,
"columnno": 0,
"code": {
- "id": "astnode100010225",
+ "id": "astnode100010221",
"name": "Horizon",
"type": "FunctionDeclaration",
"paramnames": [
@@ -20165,14 +20140,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 8,
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"value": ""
@@ -20190,14 +20165,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
"lineno": 1928,
"columnno": 10,
"code": {
- "id": "astnode100010252",
+ "id": "astnode100010248",
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"value": ""
@@ -20215,14 +20190,14 @@
"comment": "",
"meta": {
"range": [
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"comment": "/**\n * @brief Calculates the angular separation between the Sun and the given body.\n *\n * Returns the full angle seen from\n * the Earth, between the given body and the Sun.\n * Unlike {@link LongitudeFromSun}, this function does not\n * project the body's \"shadow\" onto the ecliptic;\n * the angle is measured in 3D space around the plane that\n * contains the centers of the Earth, the Sun, and `body`.\n *\n * @param {string} body\n * The name of a supported celestial body other than the Earth.\n *\n * @param {FlexibleDateTime} date\n * The time at which the angle from the Sun is to be found.\n *\n * @returns {number}\n * An angle in degrees in the range [0, 180].\n */",
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"comment": "/**\n * @brief Calculates heliocentric ecliptic longitude based on the J2000 equinox.\n *\n * @param {string} body\n * The name of a celestial body other than the Sun.\n *\n * @param {FlexibleDateTime} date\n * The date and time for which to calculate the ecliptic longitude.\n *\n * @returns {number}\n * The ecliptic longitude angle of the body in degrees measured counterclockwise around the mean\n * plane of the Earth's orbit, as seen from above the Sun's north pole.\n * Ecliptic longitude starts at 0 at the J2000\n * equinox and\n * increases in the same direction the Earth orbits the Sun.\n * The returned value is always in the range [0, 360).\n */",
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@@ -32625,14 +32600,14 @@
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"lineno": 3288,
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+ "id": "astnode100015731",
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@@ -32699,14 +32674,14 @@
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],
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@@ -32724,14 +32699,14 @@
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@@ -32749,14 +32724,14 @@
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+ "id": "astnode100015759",
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}
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@@ -32772,14 +32747,14 @@
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@@ -32795,14 +32770,14 @@
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@@ -32818,14 +32793,14 @@
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@@ -32867,14 +32842,14 @@
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@@ -32893,14 +32868,14 @@
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@@ -32919,14 +32894,14 @@
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@@ -32945,14 +32920,14 @@
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@@ -32971,14 +32946,14 @@
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@@ -32997,14 +32972,14 @@
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@@ -33023,14 +32998,14 @@
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@@ -33074,14 +33049,14 @@
"comment": "",
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],
"filename": "astronomy.js",
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@@ -33099,14 +33074,14 @@
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],
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+ "id": "astnode100015902",
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}
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@@ -33122,14 +33097,14 @@
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@@ -33174,14 +33149,14 @@
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@@ -33199,14 +33174,14 @@
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@@ -33225,14 +33200,14 @@
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@@ -33277,14 +33252,14 @@
"comment": "",
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"code": {
- "id": "astnode100015987",
+ "id": "astnode100015983",
"name": "exports.Illumination",
"type": "Identifier",
"value": "Illumination",
@@ -33301,14 +33276,14 @@
"comment": "",
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+ "id": "astnode100015988",
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@@ -33358,14 +33333,14 @@
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"value": "Planet.Earth.OrbitalPeriod"
@@ -33383,14 +33358,14 @@
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"value": "planet.OrbitalPeriod"
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+ "id": "astnode100016033",
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@@ -33433,14 +33408,14 @@
"comment": "/**\n * @brief Searches for when the Earth and a given body reach a relative ecliptic longitude separation.\n *\n * Searches for the date and time the relative ecliptic longitudes of\n * the specified body and the Earth, as seen from the Sun, reach a certain\n * difference. This function is useful for finding conjunctions and oppositions\n * of the planets. For the opposition of a superior planet (Mars, Jupiter, ..., Pluto),\n * or the inferior conjunction of an inferior planet (Mercury, Venus),\n * call with `targetRelLon` = 0. The 0 value indicates that both\n * planets are on the same ecliptic longitude line, ignoring the other planet's\n * distance above or below the plane of the Earth's orbit.\n * For superior conjunctions, call with `targetRelLon` = 180.\n * This means the Earth and the other planet are on opposite sides of the Sun.\n *\n * @param {string} body\n * The name of a planet other than the Earth.\n *\n * @param {number} targetRelLon\n * The desired angular difference in degrees between the ecliptic longitudes\n * of `body` and the Earth. Must be in the range (-180, +180].\n *\n * @param {FlexibleDateTime} startDate\n * The date and time after which to find the next occurrence of the\n * body and the Earth reaching the desired relative longitude.\n *\n * @returns {AstroTime}\n * The time when the Earth and the body next reach the specified relative longitudes.\n */",
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+ "id": "astnode100016048",
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@@ -33518,14 +33493,14 @@
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"value": "Planet[undefined]"
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@@ -33568,14 +33543,14 @@
"comment": "",
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@@ -33600,14 +33575,14 @@
"comment": "",
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@@ -33625,14 +33600,14 @@
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"comment": "",
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@@ -33675,14 +33650,14 @@
"comment": "",
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@@ -33700,14 +33675,14 @@
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"comment": "",
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@@ -33903,14 +33878,14 @@
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+ "id": "astnode100016234",
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"funcscope": "SearchRelativeLongitude",
@@ -33954,14 +33929,14 @@
"comment": "",
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"lineno": 3428,
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"code": {
- "id": "astnode100016254",
+ "id": "astnode100016250",
"name": "exports.SearchRelativeLongitude",
"type": "Identifier",
"value": "SearchRelativeLongitude",
@@ -33978,14 +33953,14 @@
"comment": "/**\n * @brief Determines the moon's phase expressed as an ecliptic longitude.\n *\n * @param {FlexibleDateTime} date\n * The date and time for which to calculate the moon's phase.\n *\n * @returns {number}\n * A value in the range [0, 360) indicating the difference\n * in ecliptic longitude between the center of the Sun and the\n * center of the Moon, as seen from the center of the Earth.\n * Certain longitude values have conventional meanings:\n *\n * * 0 = new moon\n * * 90 = first quarter\n * * 180 = full moon\n * * 270 = third quarter\n */",
"meta": {
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- "id": "astnode100016259",
+ "id": "astnode100016255",
"name": "MoonPhase",
"type": "FunctionDeclaration",
"paramnames": [
@@ -34031,14 +34006,14 @@
"comment": "",
"meta": {
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@@ -34055,14 +34030,14 @@
"comment": "/**\n * @brief Searches for the date and time that the Moon reaches a specified phase.\n *\n * Lunar phases are defined in terms of geocentric ecliptic longitudes\n * with respect to the Sun. When the Moon and the Sun have the same ecliptic\n * longitude, that is defined as a new moon. When the two ecliptic longitudes\n * are 180 degrees apart, that is defined as a full moon.\n * To enumerate quarter lunar phases, it is simpler to call\n * {@link SearchMoonQuarter} once, followed by repeatedly calling\n * {@link NextMoonQuarter}. `SearchMoonPhase` is only\n * necessary for finding other lunar phases than the usual quarter phases.\n *\n * @param {number} targetLon\n * The difference in geocentric ecliptic longitude between the Sun and Moon\n * that specifies the lunar phase being sought. This can be any value\n * in the range [0, 360). Here are some helpful examples:\n * 0 = new moon,\n * 90 = first quarter,\n * 180 = full moon,\n * 270 = third quarter.\n *\n * @param {FlexibleDateTime} dateStart\n * The beginning of the window of time in which to search.\n *\n * @param {number} limitDays\n * The floating point number of days after `dateStart`\n * that limits the window of time in which to search.\n *\n * @returns {AstroTime | null}\n * If the specified lunar phase occurs after `dateStart`\n * and before `limitDays` days after `dateStart`,\n * this function returns the date and time of the first such occurrence.\n * Otherwise, it returns `null`.\n */",
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"filename": "astronomy.js",
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"comment": "",
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"lineno": 3485,
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"code": {
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+ "id": "astnode100016276",
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@@ -34220,14 +34195,14 @@
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@@ -34296,14 +34271,14 @@
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"code": {
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+ "id": "astnode100016379",
"name": "exports.SearchMoonPhase",
"type": "Identifier",
"value": "SearchMoonPhase",
@@ -34445,14 +34420,14 @@
"comment": "/**\n * @brief A quarter lunar phase, along with when it occurs.\n *\n * @property {number} quarter\n * An integer as follows:\n * 0 = new moon,\n * 1 = first quarter,\n * 2 = full moon,\n * 3 = third quarter.\n *\n * @property {AstroTime} time\n * The date and time of the quarter lunar phase.\n */",
"meta": {
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"filename": "astronomy.js",
"lineno": 3529,
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"code": {
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"lineno": 3530,
"columnno": 4,
"code": {
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"name": "MoonQuarter",
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@@ -34529,14 +34504,14 @@
"comment": "/**\n * @brief A quarter lunar phase, along with when it occurs.\n *\n * @property {number} quarter\n * An integer as follows:\n * 0 = new moon,\n * 1 = first quarter,\n * 2 = full moon,\n * 3 = third quarter.\n *\n * @property {AstroTime} time\n * The date and time of the quarter lunar phase.\n */",
"meta": {
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"filename": "astronomy.js",
"lineno": 3529,
"columnno": 0,
"code": {
- "id": "astnode100016388",
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"comment": "",
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"lineno": 3531,
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"code": {
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"comment": "",
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@@ -34632,14 +34607,14 @@
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"name": "exports.MoonQuarter",
"type": "Identifier",
"value": "MoonQuarter",
@@ -34656,14 +34631,14 @@
"comment": "/**\n * @brief Finds the first quarter lunar phase after the specified date and time.\n *\n * The quarter lunar phases are: new moon, first quarter, full moon, and third quarter.\n * To enumerate quarter lunar phases, call `SearchMoonQuarter` once,\n * then pass its return value to {@link NextMoonQuarter} to find the next\n * `MoonQuarter`. Keep calling `NextMoonQuarter` in a loop,\n * passing the previous return value as the argument to the next call.\n *\n * @param {FlexibleDateTime} dateStart\n * The date and time after which to find the first quarter lunar phase.\n *\n * @returns {MoonQuarter}\n */",
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"name": "exports.SearchMoonQuarter",
"type": "Identifier",
"value": "SearchMoonQuarter",
@@ -34838,14 +34813,14 @@
"comment": "/**\n * @brief Finds the next quarter lunar phase in a series.\n *\n * Given a {@link MoonQuarter} object, finds the next consecutive\n * quarter lunar phase. See remarks in {@link SearchMoonQuarter}\n * for explanation of usage.\n *\n * @param {MoonQuarter} mq\n * The return value of a prior call to {@link MoonQuarter} or `NextMoonQuarter`.\n */",
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+ "id": "astnode100016496",
"name": "BodyRadiusAu",
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@@ -34959,14 +34934,14 @@
"comment": "/**\n * @brief Finds the next rise or set time for a body.\n *\n * Finds a rise or set time for the given body as\n * seen by an observer at the specified location on the Earth.\n * Rise time is defined as the moment when the top of the body\n * is observed to first appear above the horizon in the east.\n * Set time is defined as the moment the top of the body\n * is observed to sink below the horizon in the west.\n * The times are adjusted for typical atmospheric refraction conditions.\n *\n * @param {string} body\n * The name of the body to find the rise or set time for.\n *\n * @param {Observer} observer\n * Specifies the geographic coordinates and elevation above sea level of the observer.\n *\n * @param {number} direction\n * Either +1 to find rise time or -1 to find set time.\n * Any other value will cause an exception to be thrown.\n *\n * @param {FlexibleDateTime} dateStart\n * The date and time after which the specified rise or set time is to be found.\n *\n * @param {number} limitDays\n * The fractional number of days after `dateStart` that limits\n * when the rise or set time is to be found.\n *\n * @returns {AstroTime | null}\n * The date and time of the rise or set event, or null if no such event\n * occurs within the specified time window.\n */",
"meta": {
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+ "id": "astnode100016513",
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"comment": "",
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"comment": "",
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"comment": "",
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@@ -35173,14 +35148,14 @@
"comment": "",
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"filename": "astronomy.js",
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"comment": "",
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@@ -35244,14 +35219,14 @@
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@@ -35373,14 +35348,14 @@
"comment": "",
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+ "id": "astnode100016634",
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},
@@ -35396,14 +35371,14 @@
"comment": "",
"meta": {
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+ "id": "astnode100016637",
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},
@@ -35419,14 +35394,14 @@
"comment": "",
"meta": {
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@@ -35442,14 +35417,14 @@
"comment": "",
"meta": {
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"filename": "astronomy.js",
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"type": "CallExpression",
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@@ -35467,14 +35442,14 @@
"comment": "",
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"filename": "astronomy.js",
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"columnno": 8,
"code": {
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+ "id": "astnode100016649",
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},
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"comment": "/**\n * @brief Horizontal position of a body upon reaching an hour angle.\n *\n * Returns information about an occurrence of a celestial body\n * reaching a given hour angle as seen by an observer at a given\n * location on the surface of the Earth.\n *\n * @property {AstroTime} time\n * The date and time of the celestial body reaching the hour angle.\n *\n * @property {HorizontalCoordinates} hor\n * Topocentric horizontal coordinates for the body\n * at the time indicated by the `time` property.\n */",
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"comment": "/**\n * @brief Horizontal position of a body upon reaching an hour angle.\n *\n * Returns information about an occurrence of a celestial body\n * reaching a given hour angle as seen by an observer at a given\n * location on the surface of the Earth.\n *\n * @property {AstroTime} time\n * The date and time of the celestial body reaching the hour angle.\n *\n * @property {HorizontalCoordinates} hor\n * Topocentric horizontal coordinates for the body\n * at the time indicated by the `time` property.\n */",
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"comment": "/**\n * @brief Finds when a body will reach a given hour angle.\n *\n * Finds the next time the given body is seen to reach the specified\n * hour angle\n * by the given observer.\n * Providing `hourAngle` = 0 finds the next maximum altitude event (culmination).\n * Providing `hourAngle` = 12 finds the next minimum altitude event.\n * Note that, especially close to the Earth's poles, a body as seen on a given day\n * may always be above the horizon or always below the horizon, so the caller cannot\n * assume that a culminating object is visible nor that an object is below the horizon\n * at its minimum altitude.\n *\n * @param {string} body\n * The name of a celestial body other than the Earth.\n *\n * @param {Observer} observer\n * Specifies the geographic coordinates and elevation above sea level of the observer.\n *\n * @param {number} hourAngle\n * The hour angle expressed in\n * sidereal\n * hours for which the caller seeks to find the body attain.\n * The value must be in the range [0, 24).\n * The hour angle represents the number of sidereal hours that have\n * elapsed since the most recent time the body crossed the observer's local\n * meridian.\n * This specifying `hourAngle` = 0 finds the moment in time\n * the body reaches the highest angular altitude in a given sidereal day.\n *\n * @param {FlexibleDateTime} dateStart\n * The date and time after which the desired hour angle crossing event\n * is to be found.\n *\n * @returns {HourAngleEvent}\n */",
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"comment": "/**\n * @brief When the seasons change for a given calendar year.\n *\n * Represents the dates and times of the two solstices\n * and the two equinoxes in a given calendar year.\n * These four events define the changing of the seasons on the Earth.\n *\n * @property {AstroTime} mar_equinox\n * The date and time of the March equinox in the given calendar year.\n * This is the moment in March that the plane of the Earth's equator passes\n * through the center of the Sun; thus the Sun's declination\n * changes from a negative number to a positive number.\n * The March equinox defines\n * the beginning of spring in the northern hemisphere and\n * the beginning of autumn in the southern hemisphere.\n *\n * @property {AstroTime} jun_solstice\n * The date and time of the June solstice in the given calendar year.\n * This is the moment in June that the Sun reaches its most positive\n * declination value.\n * At this moment the Earth's north pole is most tilted most toward the Sun.\n * The June solstice defines\n * the beginning of summer in the northern hemisphere and\n * the beginning of winter in the southern hemisphere.\n *\n * @property {AstroTime} sep_equinox\n * The date and time of the September equinox in the given calendar year.\n * This is the moment in September that the plane of the Earth's equator passes\n * through the center of the Sun; thus the Sun's declination\n * changes from a positive number to a negative number.\n * The September equinox defines\n * the beginning of autumn in the northern hemisphere and\n * the beginning of spring in the southern hemisphere.\n *\n * @property {AstroTime} dec_solstice\n * The date and time of the December solstice in the given calendar year.\n * This is the moment in December that the Sun reaches its most negative\n * declination value.\n * At this moment the Earth's south pole is tilted most toward the Sun.\n * The December solstice defines\n * the beginning of winter in the northern hemisphere and\n * the beginning of summer in the southern hemisphere.\n */",
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@@ -36582,14 +36557,14 @@
"comment": "/**\n * @brief When the seasons change for a given calendar year.\n *\n * Represents the dates and times of the two solstices\n * and the two equinoxes in a given calendar year.\n * These four events define the changing of the seasons on the Earth.\n *\n * @property {AstroTime} mar_equinox\n * The date and time of the March equinox in the given calendar year.\n * This is the moment in March that the plane of the Earth's equator passes\n * through the center of the Sun; thus the Sun's declination\n * changes from a negative number to a positive number.\n * The March equinox defines\n * the beginning of spring in the northern hemisphere and\n * the beginning of autumn in the southern hemisphere.\n *\n * @property {AstroTime} jun_solstice\n * The date and time of the June solstice in the given calendar year.\n * This is the moment in June that the Sun reaches its most positive\n * declination value.\n * At this moment the Earth's north pole is most tilted most toward the Sun.\n * The June solstice defines\n * the beginning of summer in the northern hemisphere and\n * the beginning of winter in the southern hemisphere.\n *\n * @property {AstroTime} sep_equinox\n * The date and time of the September equinox in the given calendar year.\n * This is the moment in September that the plane of the Earth's equator passes\n * through the center of the Sun; thus the Sun's declination\n * changes from a positive number to a negative number.\n * The September equinox defines\n * the beginning of autumn in the northern hemisphere and\n * the beginning of spring in the southern hemisphere.\n *\n * @property {AstroTime} dec_solstice\n * The date and time of the December solstice in the given calendar year.\n * This is the moment in December that the Sun reaches its most negative\n * declination value.\n * At this moment the Earth's south pole is tilted most toward the Sun.\n * The December solstice defines\n * the beginning of winter in the northern hemisphere and\n * the beginning of summer in the southern hemisphere.\n */",
"meta": {
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"comment": "",
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"value": "mar_equinox",
@@ -36680,14 +36655,14 @@
"comment": "",
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@@ -36705,14 +36680,14 @@
"comment": "",
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"comment": "",
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"filename": "astronomy.js",
"lineno": 3846,
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"code": {
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"value": "dec_solstice",
@@ -36755,14 +36730,14 @@
"comment": "",
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"code": {
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"type": "Identifier",
"value": "SeasonInfo",
@@ -36779,14 +36754,14 @@
"comment": "/**\n * @brief Finds the equinoxes and solstices for a given calendar year.\n *\n * @param {number | AstroTime} year\n * The integer value or `AstroTime` object that specifies\n * the UTC calendar year for which to find equinoxes and solstices.\n *\n * @returns {SeasonInfo}\n */",
"meta": {
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"comment": "/**\n * @brief The viewing conditions of a body relative to the Sun.\n *\n * Represents the angular separation of a body from the Sun as seen from the Earth\n * and the relative ecliptic longitudes between that body and the Earth as seen from the Sun.\n *\n * @property {AstroTime} time\n * The date and time of the observation.\n *\n * @property {string} visibility\n * Either `\"morning\"` or `\"evening\"`,\n * indicating when the body is most easily seen.\n *\n * @property {number} elongation\n * The angle in degrees, as seen from the center of the Earth,\n * of the apparent separation between the body and the Sun.\n * This angle is measured in 3D space and is not projected onto the ecliptic plane.\n * When `elongation` is less than a few degrees, the body is very\n * difficult to see from the Earth because it is lost in the Sun's glare.\n * The elongation is always in the range [0, 180].\n *\n * @property {number} ecliptic_separation\n * The absolute value of the difference between the body's ecliptic longitude\n * and the Sun's ecliptic longitude, both as seen from the center of the Earth.\n * This angle measures around the plane of the Earth's orbit (the ecliptic),\n * and ignores how far above or below that plane the body is.\n * The ecliptic separation is measured in degrees and is always in the range [0, 180].\n *\n * @see {@link Elongation}\n */",
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@@ -37382,14 +37357,14 @@
"comment": "/**\n * @brief Calculates the viewing conditions of a body relative to the Sun.\n *\n * Calculates angular separation of a body from the Sun as seen from the Earth\n * and the relative ecliptic longitudes between that body and the Earth as seen from the Sun.\n * See the return type {@link ElongationEvent} for details.\n *\n * This function is helpful for determining how easy\n * it is to view a planet away from the Sun's glare on a given date.\n * It also determines whether the object is visible in the morning or evening;\n * this is more important the smaller the elongation is.\n * It is also used to determine how far a planet is from opposition, conjunction, or quadrature.\n *\n * @param {string} body\n * The name of the observed body. Not allowed to be `\"Earth\"`.\n *\n * @returns {ElongationEvent}\n */",
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@@ -37641,14 +37616,14 @@
"comment": "/**\n * @brief Finds the next time Mercury or Venus reaches maximum elongation.\n *\n * Searches for the next maximum elongation event for Mercury or Venus\n * that occurs after the given start date. Calling with other values\n * of `body` will result in an exception.\n * Maximum elongation occurs when the body has the greatest\n * angular separation from the Sun, as seen from the Earth.\n * Returns an `ElongationEvent` object containing the date and time of the next\n * maximum elongation, the elongation in degrees, and whether\n * the body is visible in the morning or evening.\n *\n * @param {string} body Either `\"Mercury\"` or `\"Venus\"`.\n * @param {FlexibleDateTime} startDate The date and time after which to search for the next maximum elongation event.\n *\n * @returns {ElongationEvent}\n */",
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"comment": "",
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"filename": "astronomy.js",
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"comment": "",
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@@ -37932,14 +37907,14 @@
"comment": "",
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@@ -37957,14 +37932,14 @@
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"comment": "",
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"comment": "",
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"comment": "",
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@@ -38126,14 +38101,14 @@
"comment": "",
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"filename": "astronomy.js",
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@@ -38151,14 +38126,14 @@
"comment": "",
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@@ -38176,14 +38151,14 @@
"comment": "",
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@@ -38201,14 +38176,14 @@
"comment": "",
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@@ -38226,14 +38201,14 @@
"comment": "",
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- "params": [
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"comment": "/**\n * @brief Given an equatorial vector, calculates equatorial angular coordinates.\n *\n * @param {Vector} vec\n * A vector in an equatorial coordinate system.\n *\n * @returns {EquatorialCoordinates}\n * Angular coordinates expressed in the same equatorial system as `vec`.\n */",
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"comment": "/**\n * @brief Converts Cartesian coordinates to spherical coordinates.\n *\n * Given a Cartesian vector, returns latitude, longitude, and distance.\n *\n * @param {Vector} vector\n * Cartesian vector to be converted to spherical coordinates.\n *\n * @returns {Spherical}\n * Spherical coordinates that are equivalent to the given vector.\n */",
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"comment": "/**\n * @brief Converts Cartesian coordinates to horizontal coordinates.\n *\n * Given a horizontal Cartesian vector, returns horizontal azimuth and altitude.\n *\n * *IMPORTANT:* This function differs from {@link SphereFromVector} in two ways:\n * - `SphereFromVector` returns a `lon` value that represents azimuth defined counterclockwise\n * from north (e.g., west = +90), but this function represents a clockwise rotation\n * (e.g., east = +90). The difference is because `SphereFromVector` is intended\n * to preserve the vector \"right-hand rule\", while this function defines azimuth in a more\n * traditional way as used in navigation and cartography.\n * - This function optionally corrects for atmospheric refraction, while `SphereFromVector` does not.\n *\n * The returned object contains the azimuth in `lon`.\n * It is measured in degrees clockwise from north: east = +90 degrees, west = +270 degrees.\n *\n * The altitude is stored in `lat`.\n *\n * The distance to the observed object is stored in `dist`,\n * and is expressed in astronomical units (AU).\n *\n * @param {Vector} vector\n * Cartesian vector to be converted to horizontal coordinates.\n *\n * @param {string} refraction\n * `\"normal\"`: correct altitude for atmospheric refraction (recommended).\n * `\"jplhor\"`: for JPL Horizons compatibility testing only; not recommended for normal use.\n * `null`: no atmospheric refraction correction is performed.\n *\n * @returns {Spherical}\n */",
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"comment": "/**\n * @brief Given apparent angular horizontal coordinates in `sphere`, calculate horizontal vector.\n *\n * @param {Spherical} sphere\n * A structure that contains apparent horizontal coordinates:\n * `lat` holds the refracted azimuth angle,\n * `lon` holds the azimuth in degrees clockwise from north,\n * and `dist` holds the distance from the observer to the object in AU.\n *\n * @param {AstroTime} time\n * The date and time of the observation. This is needed because the returned\n * vector object requires a valid time value when passed to certain other functions.\n *\n * @param {string} refraction\n * `\"normal\"`: correct altitude for atmospheric refraction (recommended).\n * `\"jplhor\"`: for JPL Horizons compatibility testing only; not recommended for normal use.\n * `null`: no atmospheric refraction correction is performed.\n *\n * @returns {Vector}\n * A vector in the horizontal system: `x` = north, `y` = west, and `z` = zenith (up).\n */",
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"comment": "/**\n * @brief Calculates the amount of \"lift\" to an altitude angle caused by atmospheric refraction.\n *\n * Given an altitude angle and a refraction option, calculates\n * the amount of \"lift\" caused by atmospheric refraction.\n * This is the number of degrees higher in the sky an object appears\n * due to the lensing of the Earth's atmosphere.\n *\n * @param {string} refraction\n * `\"normal\"`: correct altitude for atmospheric refraction (recommended).\n * `\"jplhor\"`: for JPL Horizons compatibility testing only; not recommended for normal use.\n * `null`: no atmospheric refraction correction is performed.\n *\n * @param {number} altitude\n * An altitude angle in a horizontal coordinate system. Must be a value between -90 and +90.\n *\n * @returns {number}\n * The angular adjustment in degrees to be added to the altitude angle to correct for atmospheric lensing.\n */",
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"comment": "/**\n * @brief Calculates the inverse of an atmospheric refraction angle.\n *\n * Given an observed altitude angle that includes atmospheric refraction,\n * calculate the negative angular correction to obtain the unrefracted\n * altitude. This is useful for cases where observed horizontal\n * coordinates are to be converted to another orientation system,\n * but refraction first must be removed from the observed position.\n *\n * @param {string} refraction\n * `\"normal\"`: correct altitude for atmospheric refraction (recommended).\n * `\"jplhor\"`: for JPL Horizons compatibility testing only; not recommended for normal use.\n * `null`: no atmospheric refraction correction is performed.\n *\n * @param {number} bent_altitude\n * The apparent altitude that includes atmospheric refraction.\n *\n * @returns {number}\n * The angular adjustment in degrees to be added to the\n * altitude angle to correct for atmospheric lensing.\n * This will be less than or equal to zero.\n */",
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"comment": "/**\n * @brief Applies a rotation to a vector, yielding a rotated vector.\n *\n * This function transforms a vector in one orientation to a vector\n * in another orientation.\n *\n * @param {RotationMatrix} rotation\n * A rotation matrix that specifies how the orientation of the vector is to be changed.\n *\n * @param {Vector} vector\n * The vector whose orientation is to be changed.\n *\n * @returns {Vector}\n * A vector in the orientation specified by `rotation`.\n */",
"meta": {
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"comment": "/**\n * @brief Calculates a rotation matrix from horizontal (HOR) to equatorial of-date (EQD).\n *\n * This is one of the family of functions that returns a rotation matrix\n * for converting from one orientation to another.\n * Source: HOR = horizontal system (x=North, y=West, z=Zenith).\n * Target: EQD = equatorial system, using equator of the specified date/time.\n *\n * @param {AstroTime} time\n * The date and time at which the Earth's equator applies.\n *\n * @param {Observer} observer\n * A location near the Earth's mean sea level that defines the observer's horizon.\n *\n * @returns {RotationMatrix}\n * A rotation matrix that converts HOR to EQD at `time` and for `observer`.\n */",
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"comment": "/**\n * @brief Calculates a rotation matrix from horizontal (HOR) to J2000 equatorial (EQJ).\n *\n * This is one of the family of functions that returns a rotation matrix\n * for converting from one orientation to another.\n * Source: HOR = horizontal system (x=North, y=West, z=Zenith).\n * Target: EQJ = equatorial system, using equator at the J2000 epoch.\n *\n * @param {AstroTime} time\n * The date and time of the observation.\n *\n * @param {Observer} observer\n * A location near the Earth's mean sea level that defines the observer's horizon.\n *\n * @returns {RotationMatrix}\n * A rotation matrix that converts HOR to EQD at `time` and for `observer`.\n */",
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"comment": "/**\n * @brief Calculates a rotation matrix from equatorial J2000 (EQJ) to horizontal (HOR).\n *\n * This is one of the family of functions that returns a rotation matrix\n * for converting from one orientation to another.\n * Source: EQJ = equatorial system, using the equator at the J2000 epoch.\n * Target: HOR = horizontal system.\n *\n * Use {@link HorizonFromVector} to convert the return value\n * to a traditional altitude/azimuth pair.\n *\n * @param time\n * The date and time of the desired horizontal orientation.\n *\n * @param observer\n * A location near the Earth's mean sea level that defines the observer's horizon.\n *\n * @return\n * A rotation matrix that converts EQJ to HOR at `time` and for `observer`.\n * The components of the horizontal vector are:\n * x = north, y = west, z = zenith (straight up from the observer).\n * These components are chosen so that the \"right-hand rule\" works for the vector\n * and so that north represents the direction where azimuth = 0.\n */",
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"comment": "/**\n * @brief Calculates a rotation matrix from equatorial of-date (EQD) to ecliptic J2000 (ECL).\n *\n * This is one of the family of functions that returns a rotation matrix\n * for converting from one orientation to another.\n * Source: EQD = equatorial system, using equator of date.\n * Target: ECL = ecliptic system, using equator at J2000 epoch.\n *\n * @param {AstroTime} time\n * The date and time of the source equator.\n *\n * @returns {RotationMatrix}\n * A rotation matrix that converts EQD to ECL.\n */",
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"comment": "/**\n * @brief Calculates a rotation matrix from ecliptic J2000 (ECL) to equatorial of-date (EQD).\n *\n * This is one of the family of functions that returns a rotation matrix\n * for converting from one orientation to another.\n * Source: ECL = ecliptic system, using equator at J2000 epoch.\n * Target: EQD = equatorial system, using equator of date.\n *\n * @param {AstroTime} time\n * The date and time of the desired equator.\n *\n * @returns {RotationMatrix}\n * A rotation matrix that converts ECL to EQD.\n */",
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"comment": "/**\n * @brief Calculates a rotation matrix from ecliptic J2000 (ECL) to horizontal (HOR).\n *\n * This is one of the family of functions that returns a rotation matrix\n * for converting from one orientation to another.\n * Source: ECL = ecliptic system, using equator at J2000 epoch.\n * Target: HOR = horizontal system.\n *\n * Use {@link HorizonFromVector} to convert the return value\n * to a traditional altitude/azimuth pair.\n *\n * @param {AstroTime} time\n * The date and time of the desired horizontal orientation.\n *\n * @param {Observer} observer\n * A location near the Earth's mean sea level that defines the observer's horizon.\n *\n * @returns {RotationMatrix}\n * A rotation matrix that converts ECL to HOR at `time` and for `observer`.\n * The components of the horizontal vector are:\n * x = north, y = west, z = zenith (straight up from the observer).\n * These components are chosen so that the \"right-hand rule\" works for the vector\n * and so that north represents the direction where azimuth = 0.\n */",
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"comment": "/**\n * @brief Calculates a rotation matrix from horizontal (HOR) to ecliptic J2000 (ECL).\n *\n * This is one of the family of functions that returns a rotation matrix\n * for converting from one orientation to another.\n * Source: HOR = horizontal system.\n * Target: ECL = ecliptic system, using equator at J2000 epoch.\n *\n * @param {AstroTime} time\n * The date and time of the horizontal observation.\n *\n * @param {Observer} observer\n * The location of the horizontal observer.\n *\n * @returns {RotationMatrix}\n * A rotation matrix that converts HOR to ECL.\n */",
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@@ -47061,14 +46949,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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+ "lineno": 6074,
"columnno": 4,
"code": {
- "id": "astnode100023133",
+ "id": "astnode100023101",
"name": "ConstelRot"
}
},
@@ -47083,14 +46971,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
- "lineno": 6092,
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"columnno": 4,
"code": {
- "id": "astnode100023136",
+ "id": "astnode100023104",
"name": "Epoch2000"
}
},
@@ -47105,14 +46993,14 @@
"comment": "/**\n * @brief Reports the constellation that a given celestial point lies within.\n *\n * @property {string} symbol\n * 3-character mnemonic symbol for the constellation, e.g. \"Ori\".\n *\n * @property {string} name\n * Full name of constellation, e.g. \"Orion\".\n *\n * @property {number} ra1875\n * Right ascension expressed in B1875 coordinates.\n *\n * @property {number} dec1875\n * Declination expressed in B1875 coordinates.\n */",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 0,
"code": {
- "id": "astnode100023138",
+ "id": "astnode100023106",
"name": "ConstellationInfo",
"type": "ClassDeclaration",
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@@ -47179,14 +47067,14 @@
"comment": "",
"meta": {
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"filename": "astronomy.js",
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"code": {
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+ "id": "astnode100023109",
"name": "ConstellationInfo",
"type": "MethodDefinition",
"paramnames": [
@@ -47211,14 +47099,14 @@
"comment": "/**\n * @brief Reports the constellation that a given celestial point lies within.\n *\n * @property {string} symbol\n * 3-character mnemonic symbol for the constellation, e.g. \"Ori\".\n *\n * @property {string} name\n * Full name of constellation, e.g. \"Orion\".\n *\n * @property {number} ra1875\n * Right ascension expressed in B1875 coordinates.\n *\n * @property {number} dec1875\n * Declination expressed in B1875 coordinates.\n */",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 0,
"code": {
- "id": "astnode100023138",
+ "id": "astnode100023106",
"name": "ConstellationInfo",
"type": "ClassDeclaration",
"paramnames": [
@@ -47284,14 +47172,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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"columnno": 8,
"code": {
- "id": "astnode100023150",
+ "id": "astnode100023118",
"name": "this.symbol",
"type": "Identifier",
"value": "symbol",
@@ -47309,14 +47197,14 @@
"comment": "",
"meta": {
"range": [
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+ 244002,
+ 244018
],
"filename": "astronomy.js",
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"columnno": 8,
"code": {
- "id": "astnode100023156",
+ "id": "astnode100023124",
"name": "this.name",
"type": "Identifier",
"value": "name",
@@ -47334,14 +47222,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 8,
"code": {
- "id": "astnode100023162",
+ "id": "astnode100023130",
"name": "this.ra1875",
"type": "Identifier",
"value": "ra1875",
@@ -47359,14 +47247,14 @@
"comment": "",
"meta": {
"range": [
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+ 244080
],
"filename": "astronomy.js",
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"columnno": 8,
"code": {
- "id": "astnode100023168",
+ "id": "astnode100023136",
"name": "this.dec1875",
"type": "Identifier",
"value": "dec1875",
@@ -47384,14 +47272,14 @@
"comment": "",
"meta": {
"range": [
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+ 244135
],
"filename": "astronomy.js",
- "lineno": 6116,
+ "lineno": 6099,
"columnno": 0,
"code": {
- "id": "astnode100023174",
+ "id": "astnode100023142",
"name": "exports.ConstellationInfo",
"type": "Identifier",
"value": "ConstellationInfo",
@@ -47408,14 +47296,14 @@
"comment": "/**\n * @brief Determines the constellation that contains the given point in the sky.\n *\n * Given J2000 equatorial (EQJ) coordinates of a point in the sky,\n * determines the constellation that contains that point.\n *\n * @param {number} ra\n * The right ascension (RA) of a point in the sky, using the J2000 equatorial system.\n *\n * @param {number} dec\n * The declination (DEC) of a point in the sky, using the J2000 equatorial system.\n *\n * @returns {ConstellationInfo}\n * An object that contains the 3-letter abbreviation and full name\n * of the constellation that contains the given (ra,dec), along with\n * the converted B1875 (ra,dec) for that point.\n */",
"meta": {
"range": [
- 245509,
- 247839
+ 244818,
+ 247022
],
"filename": "astronomy.js",
- "lineno": 6134,
+ "lineno": 6117,
"columnno": 0,
"code": {
- "id": "astnode100023179",
+ "id": "astnode100023147",
"name": "Constellation",
"type": "FunctionDeclaration",
"paramnames": [
@@ -47427,8 +47315,7 @@
"ra": "Constellation~ra",
"ConstelRot": "Constellation~ConstelRot",
"Epoch2000": "Constellation~Epoch2000",
- "dummyVector": "Constellation~dummyVector",
- "equ2000": "Constellation~equ2000",
+ "sph2000": "Constellation~sph2000",
"vec2000": "Constellation~vec2000",
"vec1875": "Constellation~vec1875",
"equ1875": "Constellation~equ1875",
@@ -47488,66 +47375,66 @@
"comment": "",
"meta": {
"range": [
- 245750,
- 245760
+ 245059,
+ 245069
+ ],
+ "filename": "astronomy.js",
+ "lineno": 6124,
+ "columnno": 4,
+ "code": {
+ "id": "astnode100023174",
+ "name": "ra",
+ "type": "Literal",
+ "funcscope": "Constellation",
+ "value": 24,
+ "paramnames": []
+ }
+ },
+ "undocumented": true,
+ "name": "ra",
+ "longname": "Constellation~ra",
+ "kind": "member",
+ "memberof": "Constellation",
+ "scope": "inner"
+ },
+ {
+ "comment": "",
+ "meta": {
+ "range": [
+ 245099,
+ 245109
+ ],
+ "filename": "astronomy.js",
+ "lineno": 6126,
+ "columnno": 8,
+ "code": {
+ "id": "astnode100023183",
+ "name": "ra",
+ "type": "Literal",
+ "funcscope": "Constellation",
+ "value": 24,
+ "paramnames": []
+ }
+ },
+ "undocumented": true,
+ "name": "ra",
+ "longname": "Constellation~ra",
+ "kind": "member",
+ "memberof": "Constellation",
+ "scope": "inner"
+ },
+ {
+ "comment": "",
+ "meta": {
+ "range": [
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],
"filename": "astronomy.js",
"lineno": 6141,
- "columnno": 4,
- "code": {
- "id": "astnode100023206",
- "name": "ra",
- "type": "Literal",
- "funcscope": "Constellation",
- "value": 24,
- "paramnames": []
- }
- },
- "undocumented": true,
- "name": "ra",
- "longname": "Constellation~ra",
- "kind": "member",
- "memberof": "Constellation",
- "scope": "inner"
- },
- {
- "comment": "",
- "meta": {
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"code": {
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- "name": "ra",
- "type": "Literal",
- "funcscope": "Constellation",
- "value": 24,
- "paramnames": []
- }
- },
- "undocumented": true,
- "name": "ra",
- "longname": "Constellation~ra",
- "kind": "member",
- "memberof": "Constellation",
- "scope": "inner"
- },
- {
- "comment": "",
- "meta": {
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- ],
- "filename": "astronomy.js",
- "lineno": 6158,
- "columnno": 8,
- "code": {
- "id": "astnode100023223",
+ "id": "astnode100023191",
"name": "ConstelRot",
"type": "CallExpression",
"funcscope": "Constellation",
@@ -47566,14 +47453,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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"columnno": 8,
"code": {
- "id": "astnode100023232",
+ "id": "astnode100023200",
"name": "Epoch2000",
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"comment": "/**\n * @brief Returns information about a lunar eclipse.\n *\n * Returned by {@link SearchLunarEclipse} or {@link NextLunarEclipse}\n * to report information about a lunar eclipse event.\n * When a lunar eclipse is found, it is classified as penumbral, partial, or total.\n * Penumbral eclipses are difficult to observe, because the moon is only slightly dimmed\n * by the Earth's penumbra; no part of the Moon touches the Earth's umbra.\n * Partial eclipses occur when part, but not all, of the Moon touches the Earth's umbra.\n * Total eclipses occur when the entire Moon passes into the Earth's umbra.\n *\n * The `kind` field thus holds one of the strings `\"penumbral\"`, `\"partial\"`,\n * or `\"total\"`, depending on the kind of lunar eclipse found.\n *\n * Field `peak` holds the date and time of the peak of the eclipse, when it is at its peak.\n *\n * Fields `sd_penum`, `sd_partial`, and `sd_total` hold the semi-duration of each phase\n * of the eclipse, which is half of the amount of time the eclipse spends in each\n * phase (expressed in minutes), or 0 if the eclipse never reaches that phase.\n * By converting from minutes to days, and subtracting/adding with `peak`, the caller\n * may determine the date and time of the beginning/end of each eclipse phase.\n *\n * @property {string} kind\n * The type of lunar eclipse found.\n *\n * @property {AstroTime} peak\n * The time of the eclipse at its peak.\n *\n * @property {number} sd_penum\n * The semi-duration of the penumbral phase in minutes.\n *\n * @property {number} sd_partial\n * The semi-duration of the penumbral phase in minutes, or 0.0 if none.\n *\n * @property {number} sd_total\n * The semi-duration of the penumbral phase in minutes, or 0.0 if none.\n *\n */",
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@@ -48031,14 +47893,14 @@
"comment": "/**\n * @brief Returns information about a lunar eclipse.\n *\n * Returned by {@link SearchLunarEclipse} or {@link NextLunarEclipse}\n * to report information about a lunar eclipse event.\n * When a lunar eclipse is found, it is classified as penumbral, partial, or total.\n * Penumbral eclipses are difficult to observe, because the moon is only slightly dimmed\n * by the Earth's penumbra; no part of the Moon touches the Earth's umbra.\n * Partial eclipses occur when part, but not all, of the Moon touches the Earth's umbra.\n * Total eclipses occur when the entire Moon passes into the Earth's umbra.\n *\n * The `kind` field thus holds one of the strings `\"penumbral\"`, `\"partial\"`,\n * or `\"total\"`, depending on the kind of lunar eclipse found.\n *\n * Field `peak` holds the date and time of the peak of the eclipse, when it is at its peak.\n *\n * Fields `sd_penum`, `sd_partial`, and `sd_total` hold the semi-duration of each phase\n * of the eclipse, which is half of the amount of time the eclipse spends in each\n * phase (expressed in minutes), or 0 if the eclipse never reaches that phase.\n * By converting from minutes to days, and subtracting/adding with `peak`, the caller\n * may determine the date and time of the beginning/end of each eclipse phase.\n *\n * @property {string} kind\n * The type of lunar eclipse found.\n *\n * @property {AstroTime} peak\n * The time of the eclipse at its peak.\n *\n * @property {number} sd_penum\n * The semi-duration of the penumbral phase in minutes.\n *\n * @property {number} sd_partial\n * The semi-duration of the penumbral phase in minutes, or 0.0 if none.\n *\n * @property {number} sd_total\n * The semi-duration of the penumbral phase in minutes, or 0.0 if none.\n *\n */",
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"comment": "/**\n * @ignore\n *\n * @brief Represents the relative alignment of the Earth and another body, and their respective shadows.\n *\n * This is an internal data structure used to assist calculation of\n * lunar eclipses, solar eclipses, and transits of Mercury and Venus.\n *\n * Definitions:\n *\n * casting body = A body that casts a shadow of interest, possibly striking another body.\n *\n * receiving body = A body on which the shadow of another body might land.\n *\n * shadow axis = The line passing through the center of the Sun and the center of the casting body.\n *\n * shadow plane = The plane passing through the center of a receiving body,\n * and perpendicular to the shadow axis.\n *\n * @property {AstroTime} time\n * The time associated with the shadow calculation.\n *\n * @property {number} u\n * The distance [au] between the center of the casting body and the shadow plane.\n *\n * @property {number} r\n * The distance [km] between center of receiving body and the shadow axis.\n *\n * @property {number} k\n * The umbra radius [km] at the shadow plane.\n *\n * @property {number} p\n * The penumbra radius [km] at the shadow plane.\n *\n * @property {Vector} target\n * The location in space where we are interested in determining how close a shadow falls.\n * For example, when calculating lunar eclipses, `target` would be the center of the Moon\n * expressed in geocentric coordinates. Then we can evaluate how far the center of the Earth's\n * shadow cone approaches the center of the Moon.\n * The vector components are expressed in [au].\n *\n * @property {Vector} dir\n * The direction in space that the shadow points away from the center of a shadow-casting body.\n * This vector lies on the shadow axis and points away from the Sun.\n * In other words: the direction light from the Sun would be traveling,\n * except that the center of a body (Earth, Moon, Mercury, or Venus) is blocking it.\n * The distance units do not matter, because the vector will be normalized.\n */",
"meta": {
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@@ -48403,14 +48265,14 @@
"comment": "/**\n * @ignore\n *\n * @brief Represents the relative alignment of the Earth and another body, and their respective shadows.\n *\n * This is an internal data structure used to assist calculation of\n * lunar eclipses, solar eclipses, and transits of Mercury and Venus.\n *\n * Definitions:\n *\n * casting body = A body that casts a shadow of interest, possibly striking another body.\n *\n * receiving body = A body on which the shadow of another body might land.\n *\n * shadow axis = The line passing through the center of the Sun and the center of the casting body.\n *\n * shadow plane = The plane passing through the center of a receiving body,\n * and perpendicular to the shadow axis.\n *\n * @property {AstroTime} time\n * The time associated with the shadow calculation.\n *\n * @property {number} u\n * The distance [au] between the center of the casting body and the shadow plane.\n *\n * @property {number} r\n * The distance [km] between center of receiving body and the shadow axis.\n *\n * @property {number} k\n * The umbra radius [km] at the shadow plane.\n *\n * @property {number} p\n * The penumbra radius [km] at the shadow plane.\n *\n * @property {Vector} target\n * The location in space where we are interested in determining how close a shadow falls.\n * For example, when calculating lunar eclipses, `target` would be the center of the Moon\n * expressed in geocentric coordinates. Then we can evaluate how far the center of the Earth's\n * shadow cone approaches the center of the Moon.\n * The vector components are expressed in [au].\n *\n * @property {Vector} dir\n * The direction in space that the shadow points away from the center of a shadow-casting body.\n * This vector lies on the shadow axis and points away from the Sun.\n * In other words: the direction light from the Sun would be traveling,\n * except that the center of a body (Earth, Moon, Mercury, or Venus) is blocking it.\n * The distance units do not matter, because the vector will be normalized.\n */",
"meta": {
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"comment": "/**\n * @brief Searches for a lunar eclipse.\n *\n * This function finds the first lunar eclipse that occurs after `startTime`.\n * A lunar eclipse may be penumbral, partial, or total.\n * See {@link LunarEclipseInfo} for more information.\n * To find a series of lunar eclipses, call this function once,\n * then keep calling {@link NextLunarEclipse} as many times as desired,\n * passing in the `center` value returned from the previous call.\n *\n * @param {FlexibleDateTime} date\n * The date and time for starting the search for a lunar eclipse.\n *\n * @returns {LunarEclipseInfo}\n */",
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"comment": "/**\n @brief Reports the time and geographic location of the peak of a solar eclipse.\n\n Returned by {@link SearchGlobalSolarEclipse} or {@link NextGlobalSolarEclipse}\n to report information about a solar eclipse event.\n\n Field `peak` holds the date and time of the peak of the eclipse, defined as\n the instant when the axis of the Moon's shadow cone passes closest to the Earth's center.\n\n The eclipse is classified as partial, annular, or total, depending on the\n maximum amount of the Sun's disc obscured, as seen at the peak location\n on the surface of the Earth.\n\n The `kind` field thus holds one of the strings `\"partial\"`, `\"annular\"`, or `\"total\"`.\n A total eclipse is when the peak observer sees the Sun completely blocked by the Moon.\n An annular eclipse is like a total eclipse, but the Moon is too far from the Earth's surface\n to completely block the Sun; instead, the Sun takes on a ring-shaped appearance.\n A partial eclipse is when the Moon blocks part of the Sun's disc, but nobody on the Earth\n observes either a total or annular eclipse.\n\n If `kind` is `\"total\"` or `\"annular\"`, the `latitude` and `longitude`\n fields give the geographic coordinates of the center of the Moon's shadow projected\n onto the daytime side of the Earth at the instant of the eclipse's peak.\n If `kind` has any other value, `latitude` and `longitude` are undefined and should\n not be used.\n\n @property {string} kind\n One of the following string values: `\"partial\"`, `\"annular\"`, `\"total\"`.\n\n @property {AstroTime} peak\n The date and time of the peak of the eclipse, defined as the instant\n when the axis of the Moon's shadow cone passes closest to the Earth's center.\n\n @property {number} distance\n The distance in kilometers between the axis of the Moon's shadow cone\n and the center of the Earth at the time indicated by `peak`.\n\n @property {number | undefined} latitude\n If `kind` holds `\"total\"`, the geographic latitude in degrees\n where the center of the Moon's shadow falls on the Earth at the\n time indicated by `peak`; otherwise, `latitude` holds `undefined`.\n\n @property {number | undefined} longitude\n If `kind` holds `\"total\"`, the geographic longitude in degrees\n where the center of the Moon's shadow falls on the Earth at the\n time indicated by `peak`; otherwise, `longitude` holds `undefined`.\n*/",
"meta": {
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@@ -51197,14 +51059,14 @@
"comment": "/**\n @brief Reports the time and geographic location of the peak of a solar eclipse.\n\n Returned by {@link SearchGlobalSolarEclipse} or {@link NextGlobalSolarEclipse}\n to report information about a solar eclipse event.\n\n Field `peak` holds the date and time of the peak of the eclipse, defined as\n the instant when the axis of the Moon's shadow cone passes closest to the Earth's center.\n\n The eclipse is classified as partial, annular, or total, depending on the\n maximum amount of the Sun's disc obscured, as seen at the peak location\n on the surface of the Earth.\n\n The `kind` field thus holds one of the strings `\"partial\"`, `\"annular\"`, or `\"total\"`.\n A total eclipse is when the peak observer sees the Sun completely blocked by the Moon.\n An annular eclipse is like a total eclipse, but the Moon is too far from the Earth's surface\n to completely block the Sun; instead, the Sun takes on a ring-shaped appearance.\n A partial eclipse is when the Moon blocks part of the Sun's disc, but nobody on the Earth\n observes either a total or annular eclipse.\n\n If `kind` is `\"total\"` or `\"annular\"`, the `latitude` and `longitude`\n fields give the geographic coordinates of the center of the Moon's shadow projected\n onto the daytime side of the Earth at the instant of the eclipse's peak.\n If `kind` has any other value, `latitude` and `longitude` are undefined and should\n not be used.\n\n @property {string} kind\n One of the following string values: `\"partial\"`, `\"annular\"`, `\"total\"`.\n\n @property {AstroTime} peak\n The date and time of the peak of the eclipse, defined as the instant\n when the axis of the Moon's shadow cone passes closest to the Earth's center.\n\n @property {number} distance\n The distance in kilometers between the axis of the Moon's shadow cone\n and the center of the Earth at the time indicated by `peak`.\n\n @property {number | undefined} latitude\n If `kind` holds `\"total\"`, the geographic latitude in degrees\n where the center of the Moon's shadow falls on the Earth at the\n time indicated by `peak`; otherwise, `latitude` holds `undefined`.\n\n @property {number | undefined} longitude\n If `kind` holds `\"total\"`, the geographic longitude in degrees\n where the center of the Moon's shadow falls on the Earth at the\n time indicated by `peak`; otherwise, `longitude` holds `undefined`.\n*/",
"meta": {
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"comment": "",
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"comment": "",
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"comment": "",
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"name": "exports.SearchGlobalSolarEclipse",
"type": "Identifier",
"value": "SearchGlobalSolarEclipse",
@@ -52866,14 +52728,14 @@
"comment": "/**\n * @brief Searches for the next global solar eclipse in a series.\n *\n * After using {@link SearchGlobalSolarEclipse} to find the first solar eclipse\n * in a series, you can call this function to find the next consecutive solar eclipse.\n * Pass in the `peak` value from the {@link GlobalSolarEclipseInfo} returned by the\n * previous call to `SearchGlobalSolarEclipse` or `NextGlobalSolarEclipse`\n * to find the next solar eclipse.\n *\n * @param {AstroTime} prevEclipseTime\n * A date and time near a new moon. Solar eclipse search will start at the next new moon.\n *\n * @returns {GlobalSolarEclipseInfo}\n */",
"meta": {
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],
"filename": "astronomy.js",
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"code": {
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"name": "NextGlobalSolarEclipse",
"type": "FunctionDeclaration",
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@@ -52921,14 +52783,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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"code": {
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"name": "startTime",
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"value": ""
@@ -52946,14 +52808,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"code": {
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"name": "exports.NextGlobalSolarEclipse",
"type": "Identifier",
"value": "NextGlobalSolarEclipse",
@@ -52970,14 +52832,14 @@
"comment": "/**\n * @brief Holds a time and the observed altitude of the Sun at that time.\n *\n * When reporting a solar eclipse observed at a specific location on the Earth\n * (a \"local\" solar eclipse), a series of events occur. In addition\n * to the time of each event, it is important to know the altitude of the Sun,\n * because each event may be invisible to the observer if the Sun is below\n * the horizon (i.e. it at night).\n *\n * If `altitude` is negative, the event is theoretical only; it would be\n * visible if the Earth were transparent, but the observer cannot actually see it.\n * If `altitude` is positive but less than a few degrees, visibility will be impaired by\n * atmospheric interference (sunrise or sunset conditions).\n *\n * @property {AstroTime} time\n * The date and time of the event.\n *\n * @property {number} altitude\n * The angular altitude of the center of the Sun above/below the horizon, at `time`,\n * corrected for atmospheric refraction and expressed in degrees.\n */",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 0,
"code": {
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"name": "EclipseEvent",
"type": "ClassDeclaration",
"paramnames": [
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"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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"columnno": 4,
"code": {
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"name": "EclipseEvent",
"type": "MethodDefinition",
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@@ -53054,14 +52916,14 @@
"comment": "/**\n * @brief Holds a time and the observed altitude of the Sun at that time.\n *\n * When reporting a solar eclipse observed at a specific location on the Earth\n * (a \"local\" solar eclipse), a series of events occur. In addition\n * to the time of each event, it is important to know the altitude of the Sun,\n * because each event may be invisible to the observer if the Sun is below\n * the horizon (i.e. it at night).\n *\n * If `altitude` is negative, the event is theoretical only; it would be\n * visible if the Earth were transparent, but the observer cannot actually see it.\n * If `altitude` is positive but less than a few degrees, visibility will be impaired by\n * atmospheric interference (sunrise or sunset conditions).\n *\n * @property {AstroTime} time\n * The date and time of the event.\n *\n * @property {number} altitude\n * The angular altitude of the center of the Sun above/below the horizon, at `time`,\n * corrected for atmospheric refraction and expressed in degrees.\n */",
"meta": {
"range": [
- 273271,
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],
"filename": "astronomy.js",
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"columnno": 0,
"code": {
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"name": "EclipseEvent",
"type": "ClassDeclaration",
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"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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"code": {
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"name": "this.time",
"type": "Identifier",
"value": "time",
@@ -53132,14 +52994,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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"code": {
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"name": "this.altitude",
"type": "Identifier",
"value": "altitude",
@@ -53157,14 +53019,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 0,
"code": {
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"name": "exports.EclipseEvent",
"type": "Identifier",
"value": "EclipseEvent",
@@ -53181,14 +53043,14 @@
"comment": "/**\n * @brief Information about a solar eclipse as seen by an observer at a given time and geographic location.\n *\n * Returned by {@link SearchLocalSolarEclipse} or {@link NextLocalSolarEclipse}\n * to report information about a solar eclipse as seen at a given geographic location.\n *\n * When a solar eclipse is found, it is classified by setting `kind`\n * to `\"partial\"`, `\"annular\"`, or `\"total\"`.\n * A partial solar eclipse is when the Moon does not line up directly enough with the Sun\n * to completely block the Sun's light from reaching the observer.\n * An annular eclipse occurs when the Moon's disc is completely visible against the Sun\n * but the Moon is too far away to completely block the Sun's light; this leaves the\n * Sun with a ring-like appearance.\n * A total eclipse occurs when the Moon is close enough to the Earth and aligned with the\n * Sun just right to completely block all sunlight from reaching the observer.\n *\n * There are 5 \"event\" fields, each of which contains a time and a solar altitude.\n * Field `peak` holds the date and time of the center of the eclipse, when it is at its peak.\n * The fields `partial_begin` and `partial_end` are always set, and indicate when\n * the eclipse begins/ends. If the eclipse reaches totality or becomes annular,\n * `total_begin` and `total_end` indicate when the total/annular phase begins/ends.\n * When an event field is valid, the caller must also check its `altitude` field to\n * see whether the Sun is above the horizon at the time indicated by the `time` field.\n * See {@link EclipseEvent} for more information.\n *\n * @property {string} kind\n * The type of solar eclipse found: `\"partial\"`, `\"annular\"`, or `\"total\"`.\n *\n * @property {EclipseEvent} partial_begin\n * The time and Sun altitude at the beginning of the eclipse.\n *\n * @property {EclipseEvent | undefined} total_begin\n * If this is an annular or a total eclipse, the time and Sun altitude when annular/total phase begins; otherwise undefined.\n *\n * @property {EclipseEvent} peak\n * The time and Sun altitude when the eclipse reaches its peak.\n *\n * @property {EclipseEvent | undefined} total_end\n * If this is an annular or a total eclipse, the time and Sun altitude when annular/total phase ends; otherwise undefined.\n *\n * @property {EclipseEvent} partial_end\n * The time and Sun altitude at the end of the eclipse.\n */",
"meta": {
"range": [
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],
"filename": "astronomy.js",
- "lineno": 6774,
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"columnno": 0,
"code": {
- "id": "astnode100025150",
+ "id": "astnode100025110",
"name": "LocalSolarEclipseInfo",
"type": "ClassDeclaration",
"paramnames": [
@@ -53277,14 +53139,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 4,
"code": {
- "id": "astnode100025153",
+ "id": "astnode100025113",
"name": "LocalSolarEclipseInfo",
"type": "MethodDefinition",
"paramnames": [
@@ -53311,14 +53173,14 @@
"comment": "/**\n * @brief Information about a solar eclipse as seen by an observer at a given time and geographic location.\n *\n * Returned by {@link SearchLocalSolarEclipse} or {@link NextLocalSolarEclipse}\n * to report information about a solar eclipse as seen at a given geographic location.\n *\n * When a solar eclipse is found, it is classified by setting `kind`\n * to `\"partial\"`, `\"annular\"`, or `\"total\"`.\n * A partial solar eclipse is when the Moon does not line up directly enough with the Sun\n * to completely block the Sun's light from reaching the observer.\n * An annular eclipse occurs when the Moon's disc is completely visible against the Sun\n * but the Moon is too far away to completely block the Sun's light; this leaves the\n * Sun with a ring-like appearance.\n * A total eclipse occurs when the Moon is close enough to the Earth and aligned with the\n * Sun just right to completely block all sunlight from reaching the observer.\n *\n * There are 5 \"event\" fields, each of which contains a time and a solar altitude.\n * Field `peak` holds the date and time of the center of the eclipse, when it is at its peak.\n * The fields `partial_begin` and `partial_end` are always set, and indicate when\n * the eclipse begins/ends. If the eclipse reaches totality or becomes annular,\n * `total_begin` and `total_end` indicate when the total/annular phase begins/ends.\n * When an event field is valid, the caller must also check its `altitude` field to\n * see whether the Sun is above the horizon at the time indicated by the `time` field.\n * See {@link EclipseEvent} for more information.\n *\n * @property {string} kind\n * The type of solar eclipse found: `\"partial\"`, `\"annular\"`, or `\"total\"`.\n *\n * @property {EclipseEvent} partial_begin\n * The time and Sun altitude at the beginning of the eclipse.\n *\n * @property {EclipseEvent | undefined} total_begin\n * If this is an annular or a total eclipse, the time and Sun altitude when annular/total phase begins; otherwise undefined.\n *\n * @property {EclipseEvent} peak\n * The time and Sun altitude when the eclipse reaches its peak.\n *\n * @property {EclipseEvent | undefined} total_end\n * If this is an annular or a total eclipse, the time and Sun altitude when annular/total phase ends; otherwise undefined.\n *\n * @property {EclipseEvent} partial_end\n * The time and Sun altitude at the end of the eclipse.\n */",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 0,
"code": {
- "id": "astnode100025150",
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"name": "LocalSolarEclipseInfo",
"type": "ClassDeclaration",
"paramnames": [
@@ -53406,14 +53268,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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"code": {
- "id": "astnode100025164",
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"name": "this.kind",
"type": "Identifier",
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@@ -53431,14 +53293,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"code": {
- "id": "astnode100025170",
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"name": "this.partial_begin",
"type": "Identifier",
"value": "partial_begin",
@@ -53456,14 +53318,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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"value": "total_begin",
@@ -53481,14 +53343,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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"code": {
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"name": "this.peak",
"type": "Identifier",
"value": "peak",
@@ -53506,14 +53368,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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@@ -53531,14 +53393,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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"code": {
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"name": "exports.LocalSolarEclipseInfo",
"type": "Identifier",
"value": "LocalSolarEclipseInfo",
@@ -53580,14 +53442,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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"columnno": 0,
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"type": "FunctionDeclaration",
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"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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"name": "LocalEclipse",
"type": "FunctionDeclaration",
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@@ -53671,14 +53533,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"code": {
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"type": "Literal",
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@@ -53696,14 +53558,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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@@ -53721,14 +53583,14 @@
"comment": "",
"meta": {
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],
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@@ -53746,14 +53608,14 @@
"comment": "",
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],
"filename": "astronomy.js",
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@@ -53771,14 +53633,14 @@
"comment": "",
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],
"filename": "astronomy.js",
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@@ -53796,14 +53658,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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@@ -53821,14 +53683,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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@@ -53846,14 +53708,14 @@
"comment": "",
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],
"filename": "astronomy.js",
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}
},
@@ -53869,14 +53731,14 @@
"comment": "",
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],
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}
},
@@ -53892,14 +53754,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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}
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@@ -53915,14 +53777,14 @@
"comment": "",
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],
"filename": "astronomy.js",
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"funcscope": "LocalEclipse",
@@ -53941,14 +53803,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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@@ -53967,14 +53829,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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"funcscope": "LocalEclipse",
@@ -53993,14 +53855,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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"funcscope": "LocalEclipse",
@@ -54019,14 +53881,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"funcscope": "LocalEclipse",
@@ -54045,14 +53907,14 @@
"comment": "",
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],
"filename": "astronomy.js",
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"funcscope": "LocalEclipse",
@@ -54071,14 +53933,14 @@
"comment": "",
"meta": {
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],
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@@ -54105,14 +53967,14 @@
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@@ -54135,14 +53997,14 @@
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],
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@@ -54160,14 +54022,14 @@
"comment": "",
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@@ -54185,14 +54047,14 @@
"comment": "",
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"filename": "astronomy.js",
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@@ -54215,14 +54077,14 @@
"comment": "",
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"filename": "astronomy.js",
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@@ -54240,14 +54102,14 @@
"comment": "",
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],
"filename": "astronomy.js",
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@@ -54271,14 +54133,14 @@
"comment": "",
"meta": {
"range": [
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"filename": "astronomy.js",
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@@ -54296,14 +54158,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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@@ -54321,14 +54183,14 @@
"comment": "/**\n * @brief Searches for a solar eclipse visible at a specific location on the Earth's surface.\n *\n * This function finds the first solar eclipse that occurs after `startTime`.\n * A solar eclipse may be partial, annular, or total.\n * See {@link LocalSolarEclipseInfo} for more information.\n *\n * To find a series of solar eclipses, call this function once,\n * then keep calling {@link NextLocalSolarEclipse} as many times as desired,\n * passing in the `peak` value returned from the previous call.\n *\n * IMPORTANT: An eclipse reported by this function might be partly or\n * completely invisible to the observer due to the time of day.\n * See {@link LocalSolarEclipseInfo} for more information about this topic.\n *\n * @param {AstroTime} startTime\n * The date and time for starting the search for a solar eclipse.\n *\n * @param {Observer} observer\n * The geographic location of the observer.\n *\n * @returns {LocalSolarEclipseInfo}\n */",
"meta": {
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"comment": "",
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@@ -54416,14 +54278,14 @@
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],
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@@ -54441,14 +54303,14 @@
"comment": "",
"meta": {
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],
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@@ -54466,14 +54328,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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@@ -54491,14 +54353,14 @@
"comment": "",
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],
"filename": "astronomy.js",
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"comment": "",
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],
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"comment": "",
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],
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"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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"name": "exports.SearchLocalSolarEclipse",
"type": "Identifier",
"value": "SearchLocalSolarEclipse",
@@ -54591,14 +54453,14 @@
"comment": "/**\n * @brief Searches for the next local solar eclipse in a series.\n *\n * After using {@link SearchLocalSolarEclipse} to find the first solar eclipse\n * in a series, you can call this function to find the next consecutive solar eclipse.\n * Pass in the `peak` value from the {@link LocalSolarEclipseInfo} returned by the\n * previous call to `SearchLocalSolarEclipse` or `NextLocalSolarEclipse`\n * to find the next solar eclipse.\n * This function finds the first solar eclipse that occurs after `startTime`.\n * A solar eclipse may be partial, annular, or total.\n * See {@link LocalSolarEclipseInfo} for more information.\n *\n * @param {AstroTime} prevEclipseTime\n * The date and time for starting the search for a solar eclipse.\n *\n * @param {Observer} observer\n * The geographic location of the observer.\n *\n * @returns {LocalSolarEclipseInfo}\n */",
"meta": {
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],
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"comment": "",
"meta": {
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],
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@@ -54681,14 +54543,14 @@
"comment": "",
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],
"filename": "astronomy.js",
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"comment": "/**\n * @brief Information about a transit of Mercury or Venus, as seen from the Earth.\n *\n * Returned by {@link SearchTransit} or {@link NextTransit} to report\n * information about a transit of Mercury or Venus.\n * A transit is when Mercury or Venus passes between the Sun and Earth so that\n * the other planet is seen in silhouette against the Sun.\n *\n * The calculations are performed from the point of view of a geocentric observer.\n *\n * @property {AstroTime} start\n * The date and time at the beginning of the transit.\n * This is the moment the planet first becomes visible against the Sun in its background.\n *\n * @property {AstroTime} peak\n * When the planet is most aligned with the Sun, as seen from the Earth.\n *\n * @property {AstroTime} finish\n * The date and time at the end of the transit.\n * This is the moment the planet is last seen against the Sun in its background.\n *\n * @property {number} separation\n * The minimum angular separation, in arcminutes, between the centers of the Sun and the planet.\n * This angle pertains to the time stored in `peak`.\n */",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"code": {
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+ "id": "astnode100025577",
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"comment": "/**\n * @brief Information about a transit of Mercury or Venus, as seen from the Earth.\n *\n * Returned by {@link SearchTransit} or {@link NextTransit} to report\n * information about a transit of Mercury or Venus.\n * A transit is when Mercury or Venus passes between the Sun and Earth so that\n * the other planet is seen in silhouette against the Sun.\n *\n * The calculations are performed from the point of view of a geocentric observer.\n *\n * @property {AstroTime} start\n * The date and time at the beginning of the transit.\n * This is the moment the planet first becomes visible against the Sun in its background.\n *\n * @property {AstroTime} peak\n * When the planet is most aligned with the Sun, as seen from the Earth.\n *\n * @property {AstroTime} finish\n * The date and time at the end of the transit.\n * This is the moment the planet is last seen against the Sun in its background.\n *\n * @property {number} separation\n * The minimum angular separation, in arcminutes, between the centers of the Sun and the planet.\n * This angle pertains to the time stored in `peak`.\n */",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"code": {
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@@ -54884,14 +54746,14 @@
"comment": "",
"meta": {
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],
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"code": {
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"type": "Identifier",
"value": "start",
@@ -54909,14 +54771,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 8,
"code": {
- "id": "astnode100025632",
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"name": "this.peak",
"type": "Identifier",
"value": "peak",
@@ -54934,14 +54796,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 8,
"code": {
- "id": "astnode100025638",
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"name": "this.finish",
"type": "Identifier",
"value": "finish",
@@ -54959,14 +54821,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 8,
"code": {
- "id": "astnode100025644",
+ "id": "astnode100025604",
"name": "this.separation",
"type": "Identifier",
"value": "separation",
@@ -54984,14 +54846,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 0,
"code": {
- "id": "astnode100025650",
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"name": "exports.TransitInfo",
"type": "Identifier",
"value": "TransitInfo",
@@ -55008,14 +54870,14 @@
"comment": "",
"meta": {
"range": [
- 283437,
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],
"filename": "astronomy.js",
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"columnno": 0,
"code": {
- "id": "astnode100025655",
+ "id": "astnode100025615",
"name": "PlanetShadowBoundary",
"type": "FunctionDeclaration",
"paramnames": [
@@ -55040,14 +54902,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 10,
"code": {
- "id": "astnode100025663",
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"name": "shadow",
"type": "CallExpression",
"value": ""
@@ -55065,14 +54927,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 0,
"code": {
- "id": "astnode100025680",
+ "id": "astnode100025640",
"name": "PlanetTransitBoundary",
"type": "FunctionDeclaration",
"paramnames": [
@@ -55099,14 +54961,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 10,
"code": {
- "id": "astnode100025689",
+ "id": "astnode100025649",
"name": "tx",
"type": "CallExpression",
"value": ""
@@ -55124,14 +54986,14 @@
"comment": "/**\n * @brief Searches for the first transit of Mercury or Venus after a given date.\n *\n * Finds the first transit of Mercury or Venus after a specified date.\n * A transit is when an inferior planet passes between the Sun and the Earth\n * so that the silhouette of the planet is visible against the Sun in the background.\n * To continue the search, pass the `finish` time in the returned structure to\n * {@link NextTransit}.\n *\n * @param {string} body\n * The planet whose transit is to be found. Must be `\"Mercury\"` or `\"Venus\"`.\n *\n * @param {AstroTime} startTime\n * The date and time for starting the search for a transit.\n *\n * @returns {TransitInfo}\n */",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 0,
"code": {
- "id": "astnode100025710",
+ "id": "astnode100025670",
"name": "SearchTransit",
"type": "FunctionDeclaration",
"paramnames": [
@@ -55200,14 +55062,14 @@
"comment": "",
"meta": {
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],
"filename": "astronomy.js",
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"columnno": 10,
"code": {
- "id": "astnode100025716",
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"name": "threshold_angle",
"type": "Literal",
"value": 0.4
@@ -55225,14 +55087,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 10,
"code": {
- "id": "astnode100025720",
+ "id": "astnode100025680",
"name": "dt_days",
"type": "Literal",
"value": 1
@@ -55250,14 +55112,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 8,
"code": {
- "id": "astnode100025724",
+ "id": "astnode100025684",
"name": "planet_radius_km"
}
},
@@ -55273,14 +55135,14 @@
"comment": "",
"meta": {
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+ 284164
],
"filename": "astronomy.js",
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"columnno": 12,
"code": {
- "id": "astnode100025731",
+ "id": "astnode100025691",
"name": "planet_radius_km",
"type": "Literal",
"funcscope": "SearchTransit",
@@ -55299,14 +55161,14 @@
"comment": "",
"meta": {
"range": [
- 285036,
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],
"filename": "astronomy.js",
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"columnno": 12,
"code": {
- "id": "astnode100025738",
+ "id": "astnode100025698",
"name": "planet_radius_km",
"type": "Literal",
"funcscope": "SearchTransit",
@@ -55325,14 +55187,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 8,
"code": {
- "id": "astnode100025749",
+ "id": "astnode100025709",
"name": "search_time",
"type": "Identifier",
"value": "startTime"
@@ -55350,14 +55212,14 @@
"comment": "",
"meta": {
"range": [
- 285413,
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],
"filename": "astronomy.js",
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"code": {
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"value": ""
@@ -55375,14 +55237,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"code": {
- "id": "astnode100025763",
+ "id": "astnode100025723",
"name": "conj_separation",
"type": "CallExpression",
"value": ""
@@ -55400,14 +55262,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"code": {
- "id": "astnode100025775",
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"name": "shadow",
"type": "CallExpression",
"value": ""
@@ -55425,14 +55287,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 22,
"code": {
- "id": "astnode100025792",
+ "id": "astnode100025752",
"name": "time_before",
"type": "CallExpression",
"value": ""
@@ -55450,14 +55312,14 @@
"comment": "",
"meta": {
"range": [
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],
"filename": "astronomy.js",
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"columnno": 22,
"code": {
- "id": "astnode100025803",
+ "id": "astnode100025763",
"name": "start",
"type": "CallExpression",
"value": ""
@@ -55475,14 +55337,14 @@
"comment": "",
"meta": {
"range": [
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"comment": "",
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"comment": "",
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"value": "SearchTransit",
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"comment": "/**\n * @brief Searches for the next transit of Mercury or Venus in a series.\n *\n * After calling {@link SearchTransit} to find a transit of Mercury or Venus,\n * this function finds the next transit after that.\n * Keep calling this function as many times as you want to keep finding more transits.\n *\n * @param {string} body\n * The planet whose transit is to be found. Must be `\"Mercury\"` or `\"Venus\"`.\n *\n * @param {AstroTime} prevTransitTime\n * A date and time near the previous transit.\n *\n * @returns {TransitInfo}\n */",
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